Thumbnail Icon Instruments > Solar/Space Observing Instruments > Radio Wave Detectors


Refine by Category
 
Refine by Full text

 

35 Titles Match Your Query
Showing 1 through 35 of 35
1. SHIRE Imaging Riometer, Davis, Antarctica [Riometer_SHIRE]
Mapping 38.2 MHz cosmic noise/particle precipitation in [2].7 x 7 beams 12.8 deg, ~200 x 200km at 90km altitude. A Southern Hemisphere Imaging Riometer Experiment. A joint project of the Australian ...


2. Observatory Operations - Riometer and Magnetometer Data from the Australian Antarctic Territory and Riometer Data from Macquarie Island [ASAC_527]
An analogue data acquisition system (ADAS), designed to collect time-stamped, time series data from any analogue signal is currently used to log data from the riometer, magnetic pulsations and fluxgate ...


3. Solar Geophysical Data (SGD) Reports (1955-2009) [gov.noaa.ngdc.stp.solar.solar_geophysical_data]
Solar-Geophysical Data (SGD) reports were a comprehensive compilation of many different kinds of observational data of the sun's activity and its effects on the Earth. Data from the worldwide network ...


4. SOHO/Variability of Solar Irradiance and Gravity Oscillations (VIRGO) Data Archive [SOHO_VIRGO]
The VIRGO Experiment on the ESA/NASA SOHO Mission has three types of instruments to measure total solar irradiance (TSI) with the absolute radiometers DIARAD and PMO6V, spectral solar irradiance at ...


5. Riometer (Relative Ionospheric Opacity Meter) Data [NICT_RIO_OBS]
National Institute of Information and Communications Technology has been observing the absorption of cosmic radio noise with a standard riometer (relative ionospheric opacity meter) at 30 MHz at Syowa ...


6. Imaging Riometer Observation at Syowa Station [NIPR_UAP_IRIO_SYO]
Imaging Riometer Observation at Syowa Station


7. Upper Atmosphere Physics Monitoring Observation at Syowa Station [NIPR_UAP_UAPM_SYO]
Upper Atmosphere Physics Monitoring Observation at Syowa Station


8. Japanese Antarctic Research Expedition Geoscience Survey-VLBI [NIPR_JARE_VLBI]
Japanese Antarctic Research Expedition (JARE-39) Geoscience Survey-VLBI


9. Radio and Plasma Wave Investigation (WAVES) on WIND [WIND_WAVES]
The main purpose of the Wind spacecraft is to measure the incoming solar wind, magnetic fields and particles, although early on it will also observe the Earth's foreshock region. Wind, together with ...


10. CEDAR Incoherent Scatter Radar Data Base from NCAR/HAO [INCOHERENT_SCATTER_RADAR]   PARENT DIF
The Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR) at the National Center for Atmospheric Research/High Altitude Observatory (NCAR/HAO) incoherent-radar data base was established ...


11. Coupling, Energetics, and Dynamics of Atmospheric Regions (CEDAR) Database at NCAR/HAO [CEDAR_NCAR_HAO]   CHILD DIFs
The Coupling, Energetics, and Dynamics of Atmospheric regions (CEDAR) is a program sponsored by the National Science Foundation (NSF) designed to enhance the capability of ground-based instruments ...


12. Collaborative Research: Polar Experiment Network for Geospace Upper-atmosphere Investigations (PENGUIn) - A New Vision for Global Studies [NSF-ANT03-41050]
This project involves measuring LF/MF/HF signals at ground level from remote sites in Antarctica. The primary scientific goal is to characterize natural emissions from the Earth's aurora. Several ...


13. Upper Atmospheric and Ionospheric Data [IPST_UMD_ANTARCTIC_IONOS]
The projects that operate from instrumentation at South Pole Station, and at the Arrival Heights Laboratory at McMurdo Station, examine natural phenomena occurring in the earth's atmosphere, ...


14. Upper Atmospheric and Ionospheric Data [SIENA_ANTARCTIC_IONOS]
The projects that operate from instrumentation at South Pole Station, and at the Arrival Heights Laboratory at McMurdo Station, examine natural phenomena occurring in the earth's atmosphere, ...


15. Ottawa/Penticton 2800 MHz Solar Radio Flux [FE00216]
Solar radio flux is measured from the undisturbed solar surface, developing active regions on the sun and from short-lived enhancements above the daily level. Radio ...


16. Riometer data 1994- [uk.ac.lancs.dcs-rio_kil_1]
The Kilpisj?rvi IRIS imaging riometer in northern Finland (69.05? N, 20.79? E) is supervised by Lancaster University (UK) and operated in conjunction with Sodankyl? Geophysical Observatory (SGO), ...


17. Imaging Riometer Data at Zhongshan Station, Antarctica, Year 2005 [CNNADC_2005_Zhongshan_Station_Antarctica_IMAGING_RIOMETERS_Description]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300?300 ...


18. NASA STEREO (Solar TErrestrial RElations Observatory) Data Products [NASA_STEREO_DATA_PLACEHOLDER]
[Source: NASA/GSFC Solar TErrestrial RElations Observatory (STEREO) home page, http://stereo.gsfc.nasa.gov/ ] STEREO (Solar ...


19. NOAA Space Environment Laboratory On-Line Solar and Geophysical Data [SEL-01]
The NOAA Space Environment Laboratory collects, evaluates, and distributes data relating to space plasma events, solar activity, and cosmic ray particle activity on a nearly real-time basis. Space ...


20. Solar Ground-Based Data from the Base de donnees Solaire Sol (BASS) 2000 Project [SOLAR_BASS2000]
BASS 2000 has been initiated by the Institut National des Sciences de l'Univers together with the Midi-Pyrenees Observatory, the research group "solar and stellar magnetodynamic", the ...


21. Data set of Imaging Riometer at Zhongshan Station, Antarctica,Year 2000 [2000_16-16_S_ZS_ME01_LO_O024301_001_R0_Y]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300?300 ...


22. Data set of Imaging Riometer during the 17th CHINARE in 2000-2001 [2000-2000_17-17_S_ZS_ME01_LO_O024301_001_R0_Y]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300?300 ...


23. Very Long Baseline Interferometry Data from NASA CDDIS [CDDIS_VLBI_data]
Very Long Baseline Interferometry (VLBI) is a geometric technique: it measures the time difference between the arrival at two Earth-based antennas of a radio wavefront emitted by a distant quasar. ...


24. Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) Data Archive at NASA/NSSDC and SWRI [IMAGE]
The Imager for Magnetosphere-to-Aurora Global Exploration (IMAGE) mission produced the first comprehensive global images of the plasma populations in the inner magnetosphere. IMAGE data are archived ...


25. Data set of Imaging Riometer at Zhongshan Station, Antarctica, Year 2004 [CNNADC_2004_200132366531449_2133526497_IMAGING_RIOMETERS_Dataset]
The Imaging Riometer is used to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of ...


26. Data set of Imaging Riometer at Zhongshan Station, Antarctica, Year 2002 [CNNADC_S2002_S_IR_ZS]
The Imaging Riometer is to measure cosmic noise absorption caused by ionosphere with 8 by 8 antennas. It can monitor cosmic noise absorption at ionosphere D-region with spatial dimension of 300?300 ...


27. Images in H-alpha, 80, 160, and 327 MHz, and dynamic spectrograph data from Culgoora Observatory, Australia [CULGOORA]
The Culgoora Solar Observatory is located 25 km west of the town of Narrabri, in north-west New South Wales. The observatory conducts continuous optical and radio observations of the sun every day ...


28. Ulysses Heliospheric Data [ULYSSES]
The primary mission of the Ulysses spacecraft was to characterize the heliosphere as a function of solar latitude. The periods of primary scientific interest is when Ulysses was at or higher than ...


29. Ionosphere Physics Data from Belgrano and San Martin Bases, Antarctica [JCADM_CDA_DNA_IONOSPHYSICS]
Vertical incidence ionosoundings are being performed at the Belgrano and San Martmn stations. Ionospheric cosmic noise absorption is continuously recorded at the same stations, at a frequency of ...


30. Ionospheric absorption derived by riometers measurements at 30/38.2 MHz. [ionospheric_absorption]
Cosmic noise is received at 30/38.2 MHz by a solid state riometer and dual dipole antenna at Terra Nova Bay, Italian Antarctic Base. These kind of measurements are useful to determine the ionospheric ...


31. Imaging Riometer for Ionospheric Study Data [1997-2000_S_ZS_GP01_LO_2006]
The Imaging Riometer installed at Zhongshan Station is one of the cooperative projects between the Polar Research Institute of China (PRIC) and Japan's National Institute of Polar Research (NIPR). ...


32. Global Digital Tectonic Activity Map (DTAM) from NASA/GSFC [NASA_DTAM]
A digital tectonic and volcanic map of the world was created which integrates numerous remotely sensed and GIS databases. This integrative technique made it possible to analyze data differentiated ...


33. Horizontal Deformation Velocity Map, Version 2.0 [CA_DEFORM_VEL_MAP]
[Adapted from Horizontal Deformation Velocity Map, Version 2.0 Release Notes] The velocity map, presented in the tables and figures of this report, represents an ongoing effort by the Crustal Deformation ...


34. RIOMETER DATA, IONOSPHERIC ABSORPTION [RIO-01]
Cosmic noise is received at 38.2 MHz by a solid state Riometer and dual dipole antenna at Terra Nova Bay, Italian Antarctic Base. These kind of measurements are useful to determine the ionospheric ...


35. Reference Frames and Earth Rotation by VLBI [NAOMIZSGL]
Terrestrial and celestial reference frames and the earth rotation parameters are determined from the global geodetic VLBI observations from 1984. The data include site positions at 1988, site proper ...


Showing 1 through 35 of 35
Click here for a static view of records.

Link to Web Site