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ORGANISATION
The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities. Stas Barabash (chairman, ex officio) Anders Jörle, until 2022-12-31. Maria Nilsson (Metria), until2021-12-31.
OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicDATA – IRF
Mars Express Aspera-3 data. Astrid-2 Data Plots and Analysis. Cluster EFW electric field data. Freja F3H Data Archive. For access to data from other IRF satellite instruments, contact the IRF computer group:datagruppen@irf.se.
OBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesIRF IN UPPSALA
IRF in Uppsala. The Swedish Institute of Space Physics in Uppsala is situated at Ångströmlaboratoriet and is integrated width the Institution of Physics and Astronomy at Uppsala University. SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN SpaceLab – facilities for space instrument design, qualification and testing. The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities. A key to efficient use of existing test centres and optimised test procedures is to make theseIRF I UPPSALA
Centrala funktionerStas BarabashFöreståndare+46 980 79122stas.barabash@irf.seMats AndréBiträdande föreståndare+46 18 4715913mats.andre@irfu.seAnna-Karin UkonsaariEkonomichef+46 980 79054anna-karin.ukonsaari@irf.seCecilia FlemströmPersonalchef+46 980 79065cecilia.flemstrom@irf.seCarina GunillassonRegistrator+46 980 79075registrator@irf.se.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaRWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line. The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state . The metastable state has a radiative lifetime of 107 s.ORGANISATION
The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities. Stas Barabash (chairman, ex officio) Anders Jörle, until 2022-12-31. Maria Nilsson (Metria), until2021-12-31.
OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicDATA – IRF
Mars Express Aspera-3 data. Astrid-2 Data Plots and Analysis. Cluster EFW electric field data. Freja F3H Data Archive. For access to data from other IRF satellite instruments, contact the IRF computer group:datagruppen@irf.se.
OBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesIRF IN UPPSALA
IRF in Uppsala. The Swedish Institute of Space Physics in Uppsala is situated at Ångströmlaboratoriet and is integrated width the Institution of Physics and Astronomy at Uppsala University. SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN SpaceLab – facilities for space instrument design, qualification and testing. The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities. A key to efficient use of existing test centres and optimised test procedures is to make theseIRF I UPPSALA
Centrala funktionerStas BarabashFöreståndare+46 980 79122stas.barabash@irf.seMats AndréBiträdande föreståndare+46 18 4715913mats.andre@irfu.seAnna-Karin UkonsaariEkonomichef+46 980 79054anna-karin.ukonsaari@irf.seCecilia FlemströmPersonalchef+46 980 79065cecilia.flemstrom@irf.seCarina GunillassonRegistrator+46 980 79075registrator@irf.se.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaRWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line. The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state . The metastable state has a radiative lifetime of 107 s.OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic OBSERVATORY ACTIVITIES Kiruna Atmospheric and Geophysical Observatory (KAGO) The main purpose of IRF’s observatory (Kiruna Atmospheric and Geophysical Observatory) activities is to provide society with long, unbroken time series (on time scales of 50-100 years) of measurement data from the ionosphere and the Earth’s magnetic field. The purpose of recording this data is to increase our understanding of possibleDATA – IRF
Mars Express Aspera-3 data. Astrid-2 Data Plots and Analysis. Cluster EFW electric field data. Freja F3H Data Archive. For access to data from other IRF satellite instruments, contact the IRF computer group:datagruppen@irf.se.
SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicDATA - IRF
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesVACANCIES – IRF
Vacancies. On this page we list vacancies at the Swedish Institute of Space Physics (IRF). IRF has offices in Kiruna (head office), Umeå, Uppsala and Lund. Welcome to apply for a job with us! Right now there are no vacancies to apply for! Union representatives at IRF in Kiruna. Uwe Raffalski (SACO), uwe.raffalski@irf,se, +46 980 790 21.OBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesKIRUNA
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicKIRUNA RIOGRAM
Before 25th April 2019 measurements in Kiruna was done by a riometer from La Jolla. From 25th April 30 and 38 MHz in Kiruna are extracted from RFsRio1 Wideband Spectral Riometer. ZFS BEST PRACTICES GUIDE ZFS Best Practices Guide From Siwiki Contents 1 ZFS Administration Considerations 1.1 ZFS Storage Pools Recommendations 1.1.1 System/Memory/Swap SpaceORGANISATION
The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities. Stas Barabash (chairman, ex officio) Anders Jörle, until 2022-12-31. Maria Nilsson (Metria), until2021-12-31.
OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicOBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesDATA – IRF
Mars Express Aspera-3 data. Astrid-2 Data Plots and Analysis. Cluster EFW electric field data. Freja F3H Data Archive. For access to data from other IRF satellite instruments, contact the IRF computer group:datagruppen@irf.se.
IRF IN UPPSALA
IRF in Uppsala. The Swedish Institute of Space Physics in Uppsala is situated at Ångströmlaboratoriet and is integrated width the Institution of Physics and Astronomy at Uppsala University. SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN SpaceLab – facilities for space instrument design, qualification and testing. The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities. A key to efficient use of existing test centres and optimised test procedures is to make theseIRF I UPPSALA
Centrala funktionerStas BarabashFöreståndare+46 980 79122stas.barabash@irf.seMats AndréBiträdande föreståndare+46 18 4715913mats.andre@irfu.seAnna-Karin UkonsaariEkonomichef+46 980 79054anna-karin.ukonsaari@irf.seCecilia FlemströmPersonalchef+46 980 79065cecilia.flemstrom@irf.seCarina GunillassonRegistrator+46 980 79075registrator@irf.se.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaORGANISATION
The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities. Stas Barabash (chairman, ex officio) Anders Jörle, until 2022-12-31. Maria Nilsson (Metria), until2021-12-31.
OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicOBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesDATA – IRF
Mars Express Aspera-3 data. Astrid-2 Data Plots and Analysis. Cluster EFW electric field data. Freja F3H Data Archive. For access to data from other IRF satellite instruments, contact the IRF computer group:datagruppen@irf.se.
IRF IN UPPSALA
IRF in Uppsala. The Swedish Institute of Space Physics in Uppsala is situated at Ångströmlaboratoriet and is integrated width the Institution of Physics and Astronomy at Uppsala University. SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN SpaceLab – facilities for space instrument design, qualification and testing. The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities. A key to efficient use of existing test centres and optimised test procedures is to make theseIRF I UPPSALA
Centrala funktionerStas BarabashFöreståndare+46 980 79122stas.barabash@irf.seMats AndréBiträdande föreståndare+46 18 4715913mats.andre@irfu.seAnna-Karin UkonsaariEkonomichef+46 980 79054anna-karin.ukonsaari@irf.seCecilia FlemströmPersonalchef+46 980 79065cecilia.flemstrom@irf.seCarina GunillassonRegistrator+46 980 79075registrator@irf.se.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaRWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal MassKIRUNA RIOGRAM
Before 25th April 2019 measurements in Kiruna was done by a riometer from La Jolla. From 25th April 30 and 38 MHz in Kiruna are extracted from RFsRio1 Wideband Spectral Riometer.OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicDATA – IRF
Mars Express Aspera-3 data. Astrid-2 Data Plots and Analysis. Cluster EFW electric field data. Freja F3H Data Archive. For access to data from other IRF satellite instruments, contact the IRF computer group:datagruppen@irf.se.
SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicVACANCIES – IRF
Vacancies. On this page we list vacancies at the Swedish Institute of Space Physics (IRF). IRF has offices in Kiruna (head office), Umeå, Uppsala and Lund. Welcome to apply for a job with us! Right now there are no vacancies to apply for! Union representatives at IRF in Kiruna. Uwe Raffalski (SACO), uwe.raffalski@irf,se, +46 980 790 21.EUROPLANET 2024
Europlanet 2024 – Infrastructure for Scientific Research. The Europlanet 2024 Research Infrastructure (RI) provides free access to the world’s largest collection of planetary simulation and analysis facilities, data services and tools, a ground-based observational network and programme of community support activities.OBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesKIRUNA
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicKIRUNA RIOGRAM
Before 25th April 2019 measurements in Kiruna was done by a riometer from La Jolla. From 25th April 30 and 38 MHz in Kiruna are extracted from RFsRio1 Wideband Spectral Riometer. OXYGEN FORESHOCK OF MARS (1)O+ foreshock up to > 2000 km from the bow shock. (2)O+ ≠ H+ for location (by ~1000 km), direction, and energy. (3)Narrow flow directions (both O+ and H+) ⇒ nearly along B. (4)O+ acceleration (nearly // B) starts from the magnetosheath. (5)foreshock H+ momentum = specular reflected SW momentum + foreshock O+ momentum (∆V). Summary of this event •O+ acceleration: most likely ALIS_4D PRELIMINARY WEBSITE ALIS_4D replaced ALIS from the fall of 2019 (test operations) and with regular observatory operations starting in the fall of 2020. This is a project website primarily intended for those involved in design, developement, implementation, operations and scientific usage of ALIS_4D. For official websites of the host institutes, please refer tothe
ORGANISATION
The IRF advisory council (Insynsrådet)The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities.OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicOBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesDATA – IRF
This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website.IRF IN UPPSALA
IRF in Uppsala. The Swedish Institute of Space Physics in Uppsala is situated at Ångströmlaboratoriet and is integrated width the Institution of Physics and Astronomy at Uppsala University. SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaIRF I UPPSALA
IRF i Uppsala. Postadress: Institutet för rymdfysik Box 537 751 21 Uppsala. Besöksadress: Ångströmlaboratoriet Lägerhyddsvägen 1 75237 Uppsala
RWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state .The metastable state has a radiative lifetime of 107 s. The main sources of are direct electron impact excitation of atomic oxygen:ORGANISATION
The IRF advisory council (Insynsrådet)The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities.OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicOBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesDATA – IRF
This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website.IRF IN UPPSALA
IRF in Uppsala. The Swedish Institute of Space Physics in Uppsala is situated at Ångströmlaboratoriet and is integrated width the Institution of Physics and Astronomy at Uppsala University. SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaIRF I UPPSALA
IRF i Uppsala. Postadress: Institutet för rymdfysik Box 537 751 21 Uppsala. Besöksadress: Ångströmlaboratoriet Lägerhyddsvägen 1 75237 Uppsala
RWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state .The metastable state has a radiative lifetime of 107 s. The main sources of are direct electron impact excitation of atomic oxygen:OVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicDATA – IRF
This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website. SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicVACANCIES – IRF
Union representatives at IRF in Kiruna. Uwe Raffalski (SACO), uwe.raffalski@irf,se, +46 980 790 21 Stefan Karlsson (ST), stefan.karlsson@irf.se, +46 980 790 29 Union representatives at IRF in Uppsala Thomas Leyser (SACO), Thomas.leyser@irf.se, +46 18 471 5941EUROPLANET 2024
Europlanet 2024 – Infrastructure for Scientific Research. The Europlanet 2024 Research Infrastructure (RI) provides free access to the world’s largest collection of planetary simulation and analysis facilities, data services and tools, a ground-based observational network and programme of community support activities.OBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinatesKIRUNA
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicKIRUNA RIOGRAM
Before 25th April 2019 measurements in Kiruna was done by a riometer from La Jolla. From 25th April 30 and 38 MHz in Kiruna are extracted from RFsRio1 Wideband Spectral Riometer.NACREOUS CLOUDS
DATE TIME LOCATION DIRECTION PHOTO > ( 960116 14:15 Kiruna SSW H.N > ) Photo: V.B Victoria Barabash A.C automatic camera S.D Saga Dagnesjö S.K Sheila Kirkwood Y.M Yamauchi Masatoshi H.N Hans Nilsson L.N Linda Niva A.R Anne Rechou 960116 14:15 Kiruna SSW H.N > ) Photo: V.BVictoria
ALIS_4D PRELIMINARY WEBSITE Welcome to ALIS_4D A Swedish contribution to complementary instruments for EISCAT_3D ALIS_4D replaced ALIS from the fall of 2019 (test operations) and with regular observatory operations starting in the fall of 2020. This is a project website primarily intended for those involved in design, developement, implementation, operations and scientific usage of ALIS_4D. IRF – THE SWEDISH INSTITUTE OF SPACE PHYSICS Welcome to Swedish Institute of Space Physics. A governmental research institute under the Ministry of Education. Here you can find usable resources and more information about our research and activities. Research areas. Read about the research in space physics, atmospheric physics and space technology. Knowledge bank. OBSERVATORY ACTIVITIES Kiruna Atmospheric and Geophysical Observatory (KAGO) The main purpose of IRF’s observatory (Kiruna Atmospheric and Geophysical Observatory) activities is to provide society with long, unbroken time series (on time scales of 50-100 years) of measurement data from the ionosphere and the Earth’s magnetic field. The purpose of recording this data is to increase our understanding of possibleORGANISATION
The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities. Stas Barabash (chairman, ex officio) Anders Jörle, until 2022-12-31. Maria Nilsson (Metria), until2021-12-31.
OBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinates SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN SpaceLab – facilities for space instrument design, qualification and testing. The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities. A key to efficient use of existing test centres and optimised test procedures is to make theseIRF I UPPSALA
Centrala funktionerStas BarabashFöreståndare+46 980 79122stas.barabash@irf.seMats AndréBiträdande föreståndare+46 18 4715913mats.andre@irfu.seAnna-Karin UkonsaariEkonomichef+46 980 79054anna-karin.ukonsaari@irf.seCecilia FlemströmPersonalchef+46 980 79065cecilia.flemstrom@irf.seCarina GunillassonRegistrator+46 980 79075registrator@irf.se.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaRWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line. The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state . The metastable state has a radiative lifetime of 107 s. IRF – THE SWEDISH INSTITUTE OF SPACE PHYSICS Welcome to Swedish Institute of Space Physics. A governmental research institute under the Ministry of Education. Here you can find usable resources and more information about our research and activities. Research areas. Read about the research in space physics, atmospheric physics and space technology. Knowledge bank. OBSERVATORY ACTIVITIES Kiruna Atmospheric and Geophysical Observatory (KAGO) The main purpose of IRF’s observatory (Kiruna Atmospheric and Geophysical Observatory) activities is to provide society with long, unbroken time series (on time scales of 50-100 years) of measurement data from the ionosphere and the Earth’s magnetic field. The purpose of recording this data is to increase our understanding of possibleORGANISATION
The Government has appointed the following people as members of IRF’s advisory council. IRF’s Director is the chairman of the council, which is entrusted with keeping the government informed about the institute’s activities. Stas Barabash (chairman, ex officio) Anders Jörle, until 2022-12-31. Maria Nilsson (Metria), until2021-12-31.
OBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinates SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN SpaceLab – facilities for space instrument design, qualification and testing. The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities. A key to efficient use of existing test centres and optimised test procedures is to make theseIRF I UPPSALA
Centrala funktionerStas BarabashFöreståndare+46 980 79122stas.barabash@irf.seMats AndréBiträdande föreståndare+46 18 4715913mats.andre@irfu.seAnna-Karin UkonsaariEkonomichef+46 980 79054anna-karin.ukonsaari@irf.seCecilia FlemströmPersonalchef+46 980 79065cecilia.flemstrom@irf.seCarina GunillassonRegistrator+46 980 79075registrator@irf.se.IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaRWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line. The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state . The metastable state has a radiative lifetime of 107 s. IRF – THE SWEDISH INSTITUTE OF SPACE PHYSICS Welcome to Swedish Institute of Space Physics. A governmental research institute under the Ministry of Education. Here you can find usable resources and more information about our research and activities. Research areas. Read about the research in space physics, atmospheric physics and space technology. Knowledge bank. MASTER THESES PROJECTS Basic knowledge of a programming language; the code will be mostly in Fortran. Some knowledge of physical processes in the atmosphere. Contact person: Peter Voelger, peter.voelger@irf.se. (Solar terrestrial and atmospheric research programme) Published in March 2020. Projects on hold. Here you find projects on hold.IRF IN SPACE
IRF contributed, together with Ireland and China, to the Neutral Atom Detector Unit (NUADU), designed to detect energetic neutral atoms which originate from the interaction of space plasma with the neutral gas surrounding our planet. This enabled us to visualize movement in the invisible plasma in the magnetosphere around the Earth.IRF AND EDUCATION
IRF in Kiruna contributes to the undergraduate education at the Kiruna Space Campus in collaboration with the Division of Space Engineering at the Department of Computer Science, Systems and Space Engineering at Luleå University of Technology (LTU). Among the various degrees LTU offers is a joint European Erasmus Mundus Master in space science OBSERVATORY ACTIVITIES Kiruna Atmospheric and Geophysical Observatory (KAGO) The main purpose of IRF’s observatory (Kiruna Atmospheric and Geophysical Observatory) activities is to provide society with long, unbroken time series (on time scales of 50-100 years) of measurement data from the ionosphere and the Earth’s magnetic field. The purpose of recording this data is to increase our understanding of possibleOVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicDATA – IRF
Mars Express Aspera-3 data. Astrid-2 Data Plots and Analysis. Cluster EFW electric field data. Freja F3H Data Archive. For access to data from other IRF satellite instruments, contact the IRF computer group:datagruppen@irf.se.
INVOICING – E-INVOICE – IRF Svefaktura. Invoices are created in your own financial program and sent via your invoice exchange (VAN operator) to IRF’s invoice exchange which is OpusCapita. IRF uses corporate identity number 202100-3567 in the invoice exchange as first choice and GLN-code 7340148735673 as second choice.RIOMETRAR – IRF
The riometers used at IRF are manufactured by La Jolla Sciences, California, and operate at 30Mhz and 38Mhz. They are connected to simple antennas of the type shown below and data is recorded directly on a PC at the measurement site. A copy of the data is sent inreal-time over a
IRF – THE SWEDISH INSTITUTE OF SPACE PHYSICS This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website.ORGANISATION
Organisation. IRF has its head office in Kiruna and also has activities in Umeå, Uppsala and Lund. There is a joint institute executive for all of IRF’s offices. OBSERVATORY ACTIVITIES Kiruna Atmospheric and Geophysical Observatory (KAGO) The main purpose of IRF’s observatory (Kiruna Atmospheric and Geophysical Observatory) activities is to provide society with long, unbroken time series (on time scales of 50-100 years) of measurement data from the ionosphere and the Earth’s magnetic field. The purpose of recording this data is to increase our understanding of possibleOBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinates SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities.IRF I UPPSALA
IRF i Uppsala. Postadress: Institutet för rymdfysik Box 537 751 21 Uppsala. Besöksadress: Ångströmlaboratoriet Lägerhyddsvägen 1 75237 Uppsala
IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaRWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state .The metastable state has a radiative lifetime of 107 s. The main sources of are direct electron impact excitation of atomic oxygen: IRF – THE SWEDISH INSTITUTE OF SPACE PHYSICS This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website.ORGANISATION
Organisation. IRF has its head office in Kiruna and also has activities in Umeå, Uppsala and Lund. There is a joint institute executive for all of IRF’s offices. OBSERVATORY ACTIVITIES Kiruna Atmospheric and Geophysical Observatory (KAGO) The main purpose of IRF’s observatory (Kiruna Atmospheric and Geophysical Observatory) activities is to provide society with long, unbroken time series (on time scales of 50-100 years) of measurement data from the ionosphere and the Earth’s magnetic field. The purpose of recording this data is to increase our understanding of possibleOBSERVATORY
The Swedish Institute of Space Physics (Institutet fr rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Ume, Uppsala and Lund. The main office is located in Kiruna (geographic coordinates SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic SPACELAB – IRF FACILITIES FOR SPACE INSTRUMENTATION DESIGN The development, testing and calibration of new technologies and sensors for space missions requires the accessibility of the appropriate high quality facilities.IRF I UPPSALA
IRF i Uppsala. Postadress: Institutet för rymdfysik Box 537 751 21 Uppsala. Besöksadress: Ångströmlaboratoriet Lägerhyddsvägen 1 75237 Uppsala
IRF I KIRUNA
IRF i Kiruna. Postadress: Institutet för rymdfysik Box 812 SE-981 28 Kiruna. Besök- och leveransadress: Bengt Hultqvists väg 1 SE-981 92 Kiruna. Telefon: 0980-79000 Fax: 0980-79050 E-post:irf@irf.se KartaRWC-SWEDEN - IRF
SUMMARY (Latest update 2015-05-06-09:50 CET). Solar Activity Now. Solar cycle activity level below and on the solar surface is (low max ).; Solar activity regions ( no) and a CME ( no) on the far side of the Sun are seen. Solar activity regions on eastern limb are seen: (no ).; Solar surface magnetic activity on Earthside is (high).; Solar activity in the corona, (Earth-directed Coronal Mass (F)OUR AURORAL LINES 6300Å - The auroral red line The 6300 Å emission, the ``red line'', is sometimes seen in the upper border of auroral arcs. It is emitted by atomic oxygen in its transition from the lowest excited electronic state to the atomic ground state .The metastable state has a radiative lifetime of 107 s. The main sources of are direct electron impact excitation of atomic oxygen: IRF – THE SWEDISH INSTITUTE OF SPACE PHYSICS This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website.IRF AND EDUCATION
IRF contributes with unique competence to undergraduate and postgraduate education in Sweden. Researchers and engineers from IRF contribute to space engineering courses in Kiruna and space physicscourses in Uppsala.
MASTER THESES PROJECTS Interested in a project other than those listed? Send us a mail to irf@irf.se stating your interests, when you would like to do a project, and other relevant details, including a list of names and grades of courses you have taken.; We try to match this to suitable supervisors and projects. You meet and discuss with one or more potential supervisors to see if something can be agreed.IRF IN SPACE
The Swedish Institute of Space Physics has a long and successful history of providing instruments and services for space research projects. On this page, we provide an overview of all projects from the year 1968 to 2022 where IRF participates or has participated through scientific instruments, parts, construction services orsoftware.
OBSERVATORY ACTIVITIES Kiruna Atmospheric and Geophysical Observatory (KAGO) The main purpose of IRF’s observatory (Kiruna Atmospheric and Geophysical Observatory) activities is to provide society with long, unbroken time series (on time scales of 50-100 years) of measurement data from the ionosphere and the Earth’s magnetic field. The purpose of recording this data is to increase our understanding of possibleOVERVIEW - IRF
The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic SWEDISH INSTITUTE OF SPACE PHYSICS The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographicDATA – IRF
This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website. INVOICING – E-INVOICE – IRF This is how you invoice the Swedish Institute of Space Physics (IRF) According to a new law all purchases in the public sector in Sweden should be invoiced with e-invoice.RIOMETRAR – IRF
Created by Annelie Klint Nilsson at 2016-12-14 Last modified by MatsLuspa at 2017-10-25
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2020-05-31
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