Boolean: Solar +Radio +Astronomy +ULF (28,200), monitoring +solar +ulf (96,300), "solar observations" +ulf (594), "radio astronomy" +"below 1 khz" (21),
Designing a Sky-Noise-Limited Receiver for LWA
Terms: ulf wave (21,800), ulf waves (47,100), interplanetary magnetic field (265,000), radio sky (409,000), ULF sky (8), electromagnetic sky (244), low frequency electromagnetic sky (0), ULF observatory (10),
Terms: seismo electromagnetic (9,570), seismoelectromagnetic (1,250), seismo electromagnetism (94), seismoelectromagnetism (18),
SOHO - Definitive MDI Full Disk Magnetic Field Images Level 1.8 MDI Magnetograms
Stanford - Joint Science Operations Center
Search and Download SOHO Near Realtime Data
Terms: helioseismic and magnetic imager (4,210), solar dynamics observatory (79,300), solar oscillations (70,800),
Terms: photospheric magnetic field (30,800), coronal magnetic field (55,100),
Terms: solar variability (285,000), solar variation (109,000), daily solar variability (1), daily solar variation (4), soho satellite (63,400), acrimsat (81,800),
Boolean: "solar variability" +daily (76,100), "solar variability" +hourly (6,370), "solar variability" +minute (27,500), "solar variability" +second (116,000),
Terms: solar magnetic (490,000), solar magnetism (45,600), heliomagnetism (288), heliomagnetic (3,460), heliospheric magnetic (26,400), heliospheric magnetic field (20,700), heliospheric magnetism (2),
Terms: magnetogram (259,000), magnetograph (98,500), magnetography (48,400), magnetograms (189,000), magnetographs (17,200), vector magnetograph (36,900), longitudinal magnetograph (99), solar magnetograph (1,510), solar observatory magnetograph (26), vector magnetogram (5,380), vector magnetometry (1,290),
Terms: circularly polarized light (124,000), linearly polarized light (107,000), circular polarization (482,000), linear polarization (378,000),
NASA/Marshall Solar Physics - Magnetograph
Boolean: heliospheric +magnetic +variations (89,500), heliospheric +magnetic +pulsations (10,700), heliospheric +magnetic +oscillations (45,300), heliospheric +magnetic +fluctuations (45,800),
Terms: magnetoseismology (967), magneto-seismology (1,810), solar magnetic waves (17), solar magnetic oscillations (2), helioseismology (304,000), heliophysical year (90,800), heliophysical (154,000), global solar radio flux (35), solar radio flux (47,100), helioseismic (98,400),
International Heliophysical Year - Solar magnetic waves and oscillations - Variations in the global solar radio flux during the extreme solar eruptions of October-November 2003
ULF Waves from the Ionosphere to the Outer Planets
Terms: solar radio astronomy (14,600), solar observations (159,000), radio observatory (508,000), solar monitoring (209,000), solar bursts (23,000), solar radio emissions (9,280), solar radio burst (39,500), solar radio bursts (31,300),
Boolean: solar +bursts +ulf (21,900), solar +bursts +elf (47,600), solar +bursts +vlf (25,500), solar +bursts +khz (57,100), solar +ulf +emissions (79,500),
Signatures of magnetic reconnection in solar radio observations?
Bursts of ULF noise excited by sudden changes of solar wind dynamic pressure
Multiwavelength Milky Way Intensity Scales
Terms: planetary radio astronomy (10,100), planetary radio group (81),
Terms: jupiter radio observatory (62), university of florida radio observatory (1,010), jovian radio emissions (995), jupiter radio storm predictions (3), jupiter radio storms (60), radio jove (37,800), radio jove software (28), radio jove observations (24), jupiter l-burst (33), jupiter l-bursts (10), jupiter s-burst (41), jupiter s-bursts (55),
Boolean: jupiter +burst (2,070,000), jupiter +"l-burst" (105), jupiter +"s-burst" (469), jupiter +bursts (1,210,000), jupiter +"l-bursts" (527), jupiter +"s-bursts" (1,060),
University of Florida Radio Observatory - Radio Observatory Online - Jupiter Prediction Tables -
Internet Jupiter Radio Observatory
NASA - Radio Storms on Jupiter - Jupiter rotates once every 10 hours and the cone rotates with it like a lighthouse beam. To catch a radio storm you have to know (1) when Earth will be aligned with the edge of the cone and (2) when Io is in the right position to pour electrical energy into the storm zone. This will happen a few times in the weeks ahead
Terms: galactic background radiation (760), galactic magnetic field (37,500),
NASA's Radio JOVE Project - Solar and Planetary Radio Astronomy for Schools - Radio JOVE students and amateur scientists observe and analyze natural radio emissions of Jupiter, the Sun, and our galaxy. Testing the Receiver and Antenna Together - Links
Electromagnetic field measurements in ULF-ELF-VLF [0.001 Hz–100KHz] bands
Terms: electromagnetic tomography (31,800),
Terms: microtesla nmr (15),
Superconducting Quantum Interference Devices: State of the Art and Applications
Magnetic Audio Telescope [Archive] - SpaceBanter.com