e-callisto.blogspot.com
CALLISTORadio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz
http://e-callisto.blogspot.com/
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz
http://e-callisto.blogspot.com/
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CALLISTO | e-callisto.blogspot.com Reviews
https://e-callisto.blogspot.com
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz
e-callisto.blogspot.com
CALLISTO: Mai 2013
http://e-callisto.blogspot.com/2013_05_01_archive.html
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz. Sonntag, 19. Mai 2013. New Callisto at Hvezdaren Roztoky in Slovakia. On April 30th 2013 a new Callisto spectrometer has been installed and configured at the observatory Roztoky in eastern Slovakia. The antenna is a commercial LPDA CLP-5130 followed by a low noise Mini Circuits pre-amplifier. The author with a glass of red wine after succesful installation and configuration of the instrument in a temporary shed.
CALLISTO: Juni 2015
http://e-callisto.blogspot.com/2015_06_01_archive.html
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz. Montag, 1. Juni 2015. First dual circular polarization measurement of a solar burst with the LWA at Bleien observatory. Type III solar radio burst,. Followed by a type II. Or,. May be a drifting chain of type I. Mein Profil vollständig anzeigen. Awesome Inc.-Vorlage. Powered by Blogger.
CALLISTO: Juni 2013
http://e-callisto.blogspot.com/2013_06_01_archive.html
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz. Samstag, 1. Juni 2013. Beam power pattern / raster fly map with Callisto. PSF (point spread function) or beampattern (raster fly map) of the sun measured with a 5m dish and Callisto spectrometer. Angular range = /-12° in azimuth and in elevation while tracking the sun. Angular stepsize in elevation = 0.25°. Scanning speed 1200 rpm (0.4°/s). Stoptime = 08:44:00 UT. Mein Profil vollständig anzeigen.
CALLISTO: Februar 2014
http://e-callisto.blogspot.com/2014_02_01_archive.html
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz. Samstag, 15. Februar 2014. United Nations Office for Outer Space Affairs (UNOOSA), Committee Of the Peaceful Uses of Space (COPUOS). Mein Profil vollständig anzeigen. Awesome Inc.-Vorlage. Powered by Blogger.
CALLISTO: Juni 2014
http://e-callisto.blogspot.com/2014_06_01_archive.html
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz. Donnerstag, 12. Juni 2014. 1st ligth at Bleien observatory, Switzerland with LWA. Today a Low Wavelength Antenna (LWA) was successfully installed and we already got 1st light, a nice type III burst. And here the LWA in the bushes of Bleien. Mein Profil vollständig anzeigen. Awesome Inc.-Vorlage. Powered by Blogger.
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Radioastronomy FHNW
http://soleil80.cs.technik.fhnw.ch/solarradio
Bleien Solar Radio Data. A legacy of ETH Zurich, operated by FHNW Windisch. Quicklooks of radio flares. From observations with the spectrometers Phoenix-3, Phoenix-4, and e-Callisto (including data in fits format) in various frequency ranges between 10 and 5000 MHz. Of solar radio emission from 100 to 4000 MHz observed with the spectrometer Phoenix-2. Flare observations observed with the spectrometers Phoenix-3, Phoenix-4 and e-Callisto. In various frequency ranges between 20 and 5000 MHz. Software syste...
Instruments - Rosse Solar-Terrestrial Observatory
http://www.rosseobservatory.ie/instruments
Committee on Radio Astronomy Frequencies 57th Meeting. To see the updated news on the e-Callisto network. Site location is Latitude 53 05' 38.9' North, Longitude 7 55' 12.7' West. RSTO employs other two CALLISTO receivers connected to an array of four LOFAR low frequency band (LBA) antennae. This setup aims to test the response of the LBA recording dynamic spectra from 10 to 90 MHz in both left and right circular polarizations. Ionospheric Disturbances at Very Low Frequencies. VLF receiver at the Rosse O...
Callisto Software
http://www.e-callisto.org/Software/Callisto-Software.html
Callisto Software (C for PC, Tools, Firmware, IDL, Python etc.). 1 Tools, descriptions of host software. Host software for Philips tuner CD1316LS/IV running on Windows XP, 2000, Vista, 7 (not compatible with Win 8). Host software for Philips tuner CD1316LS/IV running on Windows XP, 2000, Vista, 7 (not compatible with Win 8). Host software for Philips tuner CD1316LS/IV-3 running on Windows XP, 2000, Vista, Win 7 (not compatible with Win 8). Separate DLL used for Borland C Builder 6. Tool to generate plots...
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E-Calling Game
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E-Calling Game
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CALLISTO
Radio spectrometer to observe solar flares at low frequencies 45 MHz - 870 MHz. Samstag, 1. April 2017. 1st light low frequency Callisto OE3FLB, Austria. Nice type V solar radio burst observed with low frequency Callisto by Fritz Lensch, Austria. Mittwoch, 6. April 2016. Dual circular polarization low frequency Callisto operational in Greenland. Kristoffer Leer and Chr. Monstein behind the LWA. Observatory in Kellyville, Kangarlussuaq, Greenland. Nice type III burst. Type I burst (noise storm).
e-Callisto solar spectrometer
International Network of Solar Radio Spectrometers. Map of current distribution. Of Callisto instruments in March 2018. Update rate 15 minutes, press reload to see latest status. One dot can represent up to 5 instruments. Statistics: more than 144 instruments at more than 80 locations worldwide. Type II burst (Ooty). Of the file-names, location and frequency range ISWI Instrument Data Management Plan. Callisto direct data access. Former instruments data Ikarus and Phoenix 1978-1994. Documentation and dat...
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