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LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalDKIST INSTRUMENTS
The primary purpose of Cryo-NIRSP is the study of solar coronal magnetic fields over a large field-of-view at near- and thermal- infrared wavelengths. Cryo-NIRSP will measure the full polarization state (Stokes I, Q, U and V) of spectral lines originating on the Sunat wavelengths from
DANIEL K. INOUYE SOLAR TELESCOPE The National Science Foundation’s (NSF) Daniel K. Inouye Solar Telescope is a four-meter solar telescope on the island of Maui, Hawai’i. It’s currently the largest solar telescope in the world. With a focus on understanding the Sun’s explosive behavior, observations of magnetic fields are at the forefront of this innovative telescope.MAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORYABOUTRESEARCHPROJECTSDATA ACCESSFOR PUBLICGALLERY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalDKIST INSTRUMENTS
The primary purpose of Cryo-NIRSP is the study of solar coronal magnetic fields over a large field-of-view at near- and thermal- infrared wavelengths. Cryo-NIRSP will measure the full polarization state (Stokes I, Q, U and V) of spectral lines originating on the Sunat wavelengths from
DANIEL K. INOUYE SOLAR TELESCOPE The National Science Foundation’s (NSF) Daniel K. Inouye Solar Telescope is a four-meter solar telescope on the island of Maui, Hawai’i. It’s currently the largest solar telescope in the world. With a focus on understanding the Sun’s explosive behavior, observations of magnetic fields are at the forefront of this innovative telescope.MAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth. CONTACT US - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalDKIST INSTRUMENTS
The Visible Spectro-polarimeter (ViSP) is a slit spectrograph that expands incoming light into its components or “colors” (that are defined by the wavelength of the light components); in other words – similar to a prism – it creates a “rainbow”. In order to simultaneously pick out almost any combination of three narrow wavelength bands (approx. 1 nanometer wide) within the solarHELIOSEISMOLOGY
Helioseismology is the study of the Sun using acoustic (sound) waves. The surface of the Sun, known as the photosphere, is the point at which light can no longer penetrate, so we cannot see inside the Sun. However, the Sun is full of sound waves, bouncing off the underside of the the surface in regular patterns. Scientists have developed delicate and complex techniques to measure these sound FLARES - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation Division of Astronomical Sciences. BLOOM NEWSLETTER SIGNUP TEST The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, POTENTIAL-FIELD SOURCE-SURFACE MODELS Potential-Field Source-Surface Models. The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a model we may assume that the electric currents in the corona do not significantly influence theglobal field
AAS-238/SPD-2021: STATUS AND IMPORTANT DATES SPD is meeting jointly and virtually this year with the AAS. Based on submitted abstracts, we will have a good turnout and some greatscience.
ACTIVATE OFFICE/VISIO/PROJECT 2010 Make sure you're logged in as a user with admin privileges. Go to the Setup\Office 2010 directory and open the "Office 2010 License Key.txt" text file. Copy the license key. In your application, go to File -> Help - > Activate or change product key. Paste the license key HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORYABOUTRESEARCHPROJECTSDATA ACCESSFOR PUBLICGALLERY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world. ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
A WORKSHOP ON THE MAGNETIC FIELD SWITCHBACKS OBSERVED BY The Parker Solar Probe (PSP) team organizes a workshop to discuss observations and models of the magnetic field switchbacks observed inthe solar wind.
DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORYABOUTRESEARCHPROJECTSDATA ACCESSFOR PUBLICGALLERY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world. ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
A WORKSHOP ON THE MAGNETIC FIELD SWITCHBACKS OBSERVED BY The Parker Solar Probe (PSP) team organizes a workshop to discuss observations and models of the magnetic field switchbacks observed inthe solar wind.
DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.HELIOSEISMOLOGY
Helioseismology is the study of the Sun using acoustic (sound) waves. The surface of the Sun, known as the photosphere, is the point at which light can no longer penetrate, so we cannot see inside the Sun. However, the Sun is full of sound waves, bouncing off the underside of the the surface in regular patterns. Scientists have developed delicate and complex techniques to measure these soundNSO IN HAWAII
DKIST is located at the Haleakala High Altitude Observatories site (HO) atop Maui’s Haleakalā. The HO site, owned and managed by the University of Hawaiʻi, currently houses 6 academic and 4 space surveillance telescopes. HO is not part of Haleakala National Park. It is located on State of Hawai’i Conservation land. DANIEL K. INOUYE SOLAR TELESCOPE The National Science Foundation’s (NSF) Daniel K. Inouye Solar Telescope is a four-meter solar telescope on the island of Maui, Hawai’i. It’s currently the largest solar telescope in the world. With a focus on understanding the Sun’s explosive behavior, observations of magnetic fields are at the forefront of this innovative telescope. FLARES - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation Division of Astronomical Sciences. POTENTIAL-FIELD SOURCE-SURFACE MODELS Potential-Field Source-Surface Models. The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a model we may assume that the electric currents in the corona do not significantly influence theglobal field
IBERIAN SPACE SCIENCE SUMMER SCHOOL (I4S), 26-30 JULY On behalf of the organizers, we invite Iberian and international PhD students and young researchers to attend the Iberian Space Science Summer School (i4s).. The First edition of the Iberian Space Science Summer School aims to provide professional development for young researchers in the domain of Space Weather, with an emphasis on the fundamental science of the Sun-Earth system, ACTIVATE OFFICE/VISIO/PROJECT 2010 Make sure you're logged in as a user with admin privileges. Go to the Setup\Office 2010 directory and open the "Office 2010 License Key.txt" text file. Copy the license key. In your application, go to File -> Help - > Activate or change product key. Paste the license key SET UP CISCO ANYCONNECT Put anyconnect.noao.edu in the "Connect To:" box in the panel. Click on the "gears" symbol to the right of the "Connect To:" box and check the box for "Enable local LAN access (if configured)" and hit the Close button. Now enter your Username and Password in the appropriate boxes, and hit the "Connect" button. DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORYABOUTRESEARCHPROJECTSDATA ACCESSFOR PUBLICGALLERY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope. ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, A WORKSHOP ON THE MAGNETIC FIELD SWITCHBACKS OBSERVED BY The Parker Solar Probe (PSP) team organizes a workshop to discuss observations and models of the magnetic field switchbacks observed inthe solar wind.
DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORYABOUTRESEARCHPROJECTSDATA ACCESSFOR PUBLICGALLERY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope. ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, A WORKSHOP ON THE MAGNETIC FIELD SWITCHBACKS OBSERVED BY The Parker Solar Probe (PSP) team organizes a workshop to discuss observations and models of the magnetic field switchbacks observed inthe solar wind.
DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.NSO IN HAWAII
DKIST is located at the Haleakala High Altitude Observatories site (HO) atop Maui’s Haleakalā. The HO site, owned and managed by the University of Hawaiʻi, currently houses 6 academic and 4 space surveillance telescopes. HO is not part of Haleakala National Park. It is located on State of Hawai’i Conservation land.HELIOSEISMOLOGY
Helioseismology is the study of the Sun using acoustic (sound) waves. The surface of the Sun, known as the photosphere, is the point at which light can no longer penetrate, so we cannot see inside the Sun. However, the Sun is full of sound waves, bouncing off the underside of the the surface in regular patterns. Scientists have developed delicate and complex techniques to measure these sound DANIEL K. INOUYE SOLAR TELESCOPE The National Science Foundation’s (NSF) Daniel K. Inouye Solar Telescope is a four-meter solar telescope on the island of Maui, Hawai’i. It’s currently the largest solar telescope in the world. With a focus on understanding the Sun’s explosive behavior, observations of magnetic fields are at the forefront of this innovative telescope.ADAPTIVE OPTICS
Many important processes on the sun happen at relatively small scales. For example, massive amounts of energy are transferred throughout the solar atmosphere by “flux tubes”, which begin as small as 30 kilometers (18.6 miles) in diameter. Flux tubes can be precursors to sunspots, solar prominences, flares, and coronal mass ejections so understanding their formation and evolution is FLARES - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation Division of Astronomical Sciences. POTENTIAL-FIELD SOURCE-SURFACE MODELS Potential-Field Source-Surface Models. The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a model we may assume that the electric currents in the corona do not significantly influence theglobal field
AAS-238/SPD-2021: STATUS AND IMPORTANT DATES SPD is meeting jointly and virtually this year with the AAS. Based on submitted abstracts, we will have a good turnout and some greatscience.
ACTIVATE OFFICE/VISIO/PROJECT 2010 Make sure you're logged in as a user with admin privileges. Go to the Setup\Office 2010 directory and open the "Office 2010 License Key.txt" text file. Copy the license key. In your application, go to File -> Help - > Activate or change product key. Paste the license key SET UP CISCO ANYCONNECT Put anyconnect.noao.edu in the "Connect To:" box in the panel. Click on the "gears" symbol to the right of the "Connect To:" box and check the box for "Enable local LAN access (if configured)" and hit the Close button. Now enter your Username and Password in the appropriate boxes, and hit the "Connect" button. HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORYABOUTRESEARCHPROJECTSDATA ACCESSFOR PUBLICGALLERY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world. ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
A WORKSHOP ON THE MAGNETIC FIELD SWITCHBACKS OBSERVED BY The Parker Solar Probe (PSP) team organizes a workshop to discuss observations and models of the magnetic field switchbacks observed inthe solar wind.
DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORYABOUTRESEARCHPROJECTSDATA ACCESSFOR PUBLICGALLERY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world. ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope.CURRENT IMAGES
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves, WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
A WORKSHOP ON THE MAGNETIC FIELD SWITCHBACKS OBSERVED BY The Parker Solar Probe (PSP) team organizes a workshop to discuss observations and models of the magnetic field switchbacks observed inthe solar wind.
DOCUMENT AND DRAWING CONTROL PLAN Document and Drawing Control Plan SPEC-0002, Rev H Page 3 of 33 1.3 SYSTEMS DATABASE The Systems Librarian maintains a Systems Database in Access. This database is accessible by the staff ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth. VIRTUAL SOLAR OBSERVATORY Virtual Solar Observatory. The Virtual Solar Observatory (VSO) project is led by Dr Frank Hill at NSO. VSO is a research tool that allows scientists to search for solar and heliospheric physics data. Users search existing databases for terrestrial and space-based observations, hiding the details of where the data is and what’sneeded to get it.
HELIOSEISMOLOGY
Helioseismology is the study of the Sun using acoustic (sound) waves. The surface of the Sun, known as the photosphere, is the point at which light can no longer penetrate, so we cannot see inside the Sun. However, the Sun is full of sound waves, bouncing off the underside of the the surface in regular patterns. Scientists have developed delicate and complex techniques to measure these soundNSO IN HAWAII
DKIST is located at the Haleakala High Altitude Observatories site (HO) atop Maui’s Haleakalā. The HO site, owned and managed by the University of Hawaiʻi, currently houses 6 academic and 4 space surveillance telescopes. HO is not part of Haleakala National Park. It is located on State of Hawai’i Conservation land. DANIEL K. INOUYE SOLAR TELESCOPE The National Science Foundation’s (NSF) Daniel K. Inouye Solar Telescope is a four-meter solar telescope on the island of Maui, Hawai’i. It’s currently the largest solar telescope in the world. With a focus on understanding the Sun’s explosive behavior, observations of magnetic fields are at the forefront of this innovative telescope.ADAPTIVE OPTICS
Many important processes on the sun happen at relatively small scales. For example, massive amounts of energy are transferred throughout the solar atmosphere by “flux tubes”, which begin as small as 30 kilometers (18.6 miles) in diameter. Flux tubes can be precursors to sunspots, solar prominences, flares, and coronal mass ejections so understanding their formation and evolution is FLARES - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation Division of Astronomical Sciences. POTENTIAL-FIELD SOURCE-SURFACE MODELS Potential-Field Source-Surface Models. The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a model we may assume that the electric currents in the corona do not significantly influence theglobal field
ACTIVATE OFFICE/VISIO/PROJECT 2010 Make sure you're logged in as a user with admin privileges. Go to the Setup\Office 2010 directory and open the "Office 2010 License Key.txt" text file. Copy the license key. In your application, go to File -> Help - > Activate or change product key. Paste the license key SET UP CISCO ANYCONNECT Put anyconnect.noao.edu in the "Connect To:" box in the panel. Click on the "gears" symbol to the right of the "Connect To:" box and check the box for "Enable local LAN access (if configured)" and hit the Close button. Now enter your Username and Password in the appropriate boxes, and hit the "Connect" button.LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope. CONTACT US - NSO - NATIONAL SOLAR OBSERVATORYNATIONAL SOLAR OBSERVATORY HAWAIINATIONAL SOLAR OBSERVATORY MAUINEW MEXICO SOLAR OBSERVATORYNATIONAL OBSERVATORY TIMENATIONAL SOLAR OBSERVATORYSACRAMENTO PEAK
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National DKIST - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalHELIOSEISMOLOGY
Helioseismology is the study of the Sun using acoustic (sound) waves. The surface of the Sun, known as the photosphere, is the point at which light can no longer penetrate, so we cannot see inside the Sun. However, the Sun is full of sound waves, bouncing off the underside of the the surface in regular patterns. Scientists have developed delicate and complex techniques to measure these soundMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
POTENTIAL-FIELD SOURCE-SURFACE MODELS Potential-Field Source-Surface Models. The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a model we may assume that the electric currents in the corona do not significantly influence theglobal field
MARK WARNER
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National OBITUARY: RICHARD SCHWARTZ (1952-2020) Obituary: Richard Schwartz (1952-2020) Richard Schwartz died unexpectedly at his home on Saturday, 12 December. Although he had been sick for over a month, he was preparing to begin chemotherapy for Non-Hodgkin’s lymphoma, so his sudden passing was a great shock. Richard got a BS from Carnegie-Mellon University in 1974 and a PhDfrom the
LATEST NEWS
Inouye Solar Telescope’s Critical Science Plan released. “Critical Science Plan for the Daniel K . Inouye Solar Telescope (DKIST),” has been published in the journal of Solar Physics. This document outlines the scientific context of the Inouye Solar Telescope, and explores the scientific objectives that will motivate the use of the telescope. CONTACT US - NSO - NATIONAL SOLAR OBSERVATORYNATIONAL SOLAR OBSERVATORY HAWAIINATIONAL SOLAR OBSERVATORY MAUINEW MEXICO SOLAR OBSERVATORYNATIONAL OBSERVATORY TIMENATIONAL SOLAR OBSERVATORYSACRAMENTO PEAK
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National DKIST - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalHELIOSEISMOLOGY
Helioseismology is the study of the Sun using acoustic (sound) waves. The surface of the Sun, known as the photosphere, is the point at which light can no longer penetrate, so we cannot see inside the Sun. However, the Sun is full of sound waves, bouncing off the underside of the the surface in regular patterns. Scientists have developed delicate and complex techniques to measure these soundMAGNETOGRAMS
Magnetograms. A magnetogram is an image taken by an instrument (magnetograph) that shows the strength, polarity, and location of the magnetic fields on the Sun. In a grayscale magnetogram, regions of strong magnetic field (active regions) are shown as white (positive polarity, magnetic field lines coming toward the observer) and black(negative
NSO: GLOBAL OSCILLATION NETWORK GROUP (GONG) Network Monitor. Venus Transit 2012. Far Side. H-alpha. NSO Workshop #27. Fifty Years of Seismology of the Sun and Stars. May 6-10, 2013. WELCOME TO THE DKIST Welcome to the DKIST. The Daniel K. Inouye Solar Telescope (DKIST, formerly the Advanced Technology Solar Telescope, ATST) represents a collaboration of 22 institutions, reflecting a broad segment of the solar physics community. The construction phase of the project, to build the next generation ground-based solar telescope, is underwaynow.
POTENTIAL-FIELD SOURCE-SURFACE MODELS Potential-Field Source-Surface Models. The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a model we may assume that the electric currents in the corona do not significantly influence theglobal field
MARK WARNER
The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National OBITUARY: RICHARD SCHWARTZ (1952-2020) Obituary: Richard Schwartz (1952-2020) Richard Schwartz died unexpectedly at his home on Saturday, 12 December. Although he had been sick for over a month, he was preparing to begin chemotherapy for Non-Hodgkin’s lymphoma, so his sudden passing was a great shock. Richard got a BS from Carnegie-Mellon University in 1974 and a PhDfrom the
HOME PAGE - NSO - NATIONAL SOLAR OBSERVATORY The NSF's National Solar Observatory's mission is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth.. NSO operates the Inouye Solar Telescope, the largest and most advanced solar telescope in the world. ABOUT - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory is a public research institute headquartered in Boulder, Colorado with a satellite facility in Maui, Hawaiʻi. The mission of NSO is to advance our understanding of the Sun, both as a star and as a major influence for life on Earth. DKIST - NSO - NATIONAL SOLAR OBSERVATORY The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NationalHELIOSEISMOLOGY
Helioseismology is the study of the Sun using acoustic (sound) waves. The surface of the Sun, known as the photosphere, is the point at which light can no longer penetrate, so we cannot see inside the Sun. However, the Sun is full of sound waves, bouncing off the underside of the the surface in regular patterns. Scientists have developed delicate and complex techniques to measure these soundNSO IN HAWAII
DKIST is located at the Haleakala High Altitude Observatories site (HO) atop Maui’s Haleakalā. The HO site, owned and managed by the University of Hawaiʻi, currently houses 6 academic and 4 space surveillance telescopes. HO is not part of Haleakala National Park. It is located on State of Hawai’i Conservation land. MOUNT WILSON OBSERVATORY HK PROJECT The Mount Wilson Observatory HK Project, which aimed at studying stellar chromospheric activity and variability, was started by Olin Wilson in early 1966 and continued by Art Vaughan, George Preston, Douglas Duncan, Sallie Baliunas, and many others through 2002, when the final observations were made (e.g., Wilson 1978, ApJ 226, pp. 379-396; Vaughan, Preston, and Wilson 1978, PASP 90, pp. 267 POTENTIAL-FIELD SOURCE-SURFACE MODELS Potential-Field Source-Surface Models. The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a model we may assume that the electric currents in the corona do not significantly influence theglobal field
SOLARNEWS | THE NEWSLETTER OF THE AAS SOLAR PHYSICS DIVISION The scientific programme of the meeting is divided into 5 separate sessions: Solar interior, dynamo, large-scale flows and the solar cycle. The solar atmosphere: heating, dynamics and coupling. Fundamental plasma processes in the solar atmosphere: magnetic reconnection, waves,IMAGE GALLERIES
Telescope Structure Complete. July 2017 TMA Status. Installing the TMA's OSS. Altitude Motor Installation. Coudé Instrument Rack Frames installed. Mount Bearing Radial Alignment Process. TMA Progress - Coudé Encoder Tape Fitting Complete. Cable Wrap Spider and Gear. Telescope Mount Base Grouting Complete. LATEST BONGO MIX 2021 MP3 DOWNLOAD GET (45:54) (63.03 MB Download Latest Bongo Mix 2021 Mp3 Download MP3 secara gratis di Dstsvcx nso. Detail Dj B TheSpinDokta: Bongo 2021:Wasafi,Zuchu,Sukari Diamond,Mbosso,Rayvanny,Otile,Nadia,Tanasha@ppp_tv MP3 dapat kamu nikmati dengan cara klik link download dibawah dengan mudah tanpa adanya iklan yang mengganggu.LATEST NEWS:
NSF’s National Solar Observatory Predicts a Large Sunspot forThanksgiving
NSO Scientists predict a large sunspot for Thanksgiving How the NSO predicted a new sunspot group before it rotated into view Community Response to the DKIST Cycle 1 Call for Proposals “Becoming a Super Solar Scientist!” – NSO WISER Live Stream for Planets Foundation’s AstroFest*
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NSF’S NATIONAL SOLAR OBSERVATORY PREDICTS A LARGE SUNSPOT FORTHANKSGIVING
NSO SCIENTISTS PREDICT A LARGE SUNSPOT FOR THANKSGIVING HOW THE NSO PREDICTED A NEW SUNSPOT GROUP BEFORE IT ROTATED INTO VIEW COMMUNITY RESPONSE TO THE DKIST CYCLE 1 CALL FOR PROPOSALS “BECOMING A SUPER SOLAR SCIENTIST!” – NSO WISER LIVE STREAM FOR PLANETS FOUNDATION’S ASTROFEST NSO SCIENTISTS PARTICIPATE IN CELEBRATION OF THE 25TH ANNIVERSARY OF GONG AT THE UDAIPUR SOLAR OBSERVATORY IN INDIA SUNSPOT CYCLE IS STABILIZING, ACCORDING TO WORLDWIDE PANEL OF EXPERTS NSO ASTRONOMERS TO PLAY KEY ROLE IN TWO NEW SPACECRAFT MISSION CONCEPTSTUDIES
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DR. THOMAS RIMMELE, DIRECTOR OF NSF’S INOUYE SOLAR TELESCOPE, NAMED ONE OF FAST COMPANY’S MOST CREATIVE PEOPLE IN BUSINESS DUNN SOLAR TELESCOPE CATCHES AN ERUPTING FILAMENTSOCIAL
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A week after NSO scientists "heard" a large sunspot on the far side of the Sun using the @nsfgov and @NOAA funded #GONG network, the sunspot has finally peeked around the edge of the Sun and is visible from Earth️
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A week after NSO scientists "heard" a large sunspot on the far side of the Sun using the @NSF and @NOAAfunded #GONG
network, the sunspot has finally peeked around the edge of the Sun and is visible from Earth☀️👀🌎
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The National Solar Observatory (NSO) is the national center for ground-based solar physics in the United States (www.nso.edu) and is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation Division of Astronomical Sciences. The National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future. Please refer to www.nsf.gov .OTHER AURA CENTERS
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nationalsolarobservatory A week after NSO scientists "heard" a large sunspot on the far side of the Sun using the @nsfgov and @NOAA funded #GONG network, the sunspot has finally peeked around the edge of the Sun and is visible from Earth️
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A week after NSO scientists "heard" a large sunspot on the far side of the Sun using the @NSF and @NOAAfunded #GONG
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