Boolean: "Electrical Grids" +"Solar Storms" (1,880), "electromagnetic noise" +"electric power" (8,370), "electromagnetic noise" +"transmission lines" (7,080), "electromagnetic noise" +"power lines" (10,100),
Boolean: "power surges" +statistics (69,100), "power surges" +monitoring (184,000),
Terms: magnetic shielding (746,000), skin effect (697,000), skin depth (311,000), propagation constant (122,000),
Terms: low frequency magnetic fields (84,500), TEM waves (13,400), transverse electromagnetic (68,100), TM waves (14,700), TE waves (10,200), electromagnetic waves in plasma (1,330), waves in plasma (25,300),
Non-Relativistic Electrodynamics
Princeton - Magnetostatic Spin Waves
Terms: magnetostatic spin waves (1,160), magnetization waves (314), spin waves (145,000), magnetostatic modes (6,300),
Terms: plasma waves (240,000), plasma oscillation (22,200), langmuir wave (18,100), upper hybrid oscillation (93), ion acoustic wave (19,600), electrostatic wave (16,400), ion cyclotron wave (11,700), o wave (160,000), x wave (202,000), r wave (321,000), l wave (63,700), magnetosonic wave (10,600), magnetostatic wave (7,320), magnetostatic waves (11,300),
Electromagnetic shielding - For static or slowly varying magnetic fields (below about 100 KHz) the Faraday shielding described above is ineffective. Also, most conductors exhibit a ferromagnetic response to low-frequency magnetic fields, so that such fields are not fully attenuated by the conductor. Skin depth,
Terms: geomagnetic disturbances (68,200), geomagnetic disturbance (41,200), geomagnetic disruption (30), geomagnetic induced currents (432), earth currents (49,900), substorm (280,000), substorms (307,000), electromagnetic noise (215,000),
Boolean: "electromagnetic interference" +geomagnetic (7,290), "solar storms" +electromagnetic +pulse (3,330), substorms +electromagnetic pulse (12,700), "electromagnetic interference" +"solar storms" (508),
Terms: electromagnetic interference (2,710,000), electromagnetic shielding (250,000), electromagnetic pulse (1,060,000), submarine electromagnetic (745), underwater electromagnetic (15,900), electromagnetic environmental (51,100), electronic shielding (25,900), magnetic pulse (486,000), electromagnetic vulnerability (2,570), geo-electromagnetic (1,750), electromagnetic bombs (10,900), electromagnetic warfare (31,100),
Navy - Electromagnetic Interference
Electromagnetic Pulse Threats in 2010
Boolean: site:mil +"electromagnetic interference" (14,000), site:mil +geomagnetic (1,490), site:mil +substorms (34), site:mil +todd +conley +electromagnetic (11), site:mil +electromagnetic (132,000),
Geomagnetic Induced Currents - During severe geomagnetic storms, values of 2 to 10 volts per mile can be induced in transmission lines with corresponding GICs in excess of 100 amperes. The frequency of GICs is very low (one to a few milliHertz) compared to our normal line frequency of 60 Hertz.
Boolean: "electric grid" +"solar storms" (1,020), "electric grid" +geomagnetic (1,220), "electric grid" +geomagnetic +(pulsation OR pulsations) (10), "electric grid" +"space weather" (1,530), geomagnetic +"earth currents" (2,770), lightning +"earth currents" (3,860), lightning +induced +"power grids" (3,100), geomagnetic +"power lines" (56,300), geomagnetic +"transmission lines" (28,400), substorm +"electric power" (1,260), substorms +"electric power" (1,630), (substorm OR substorms) +"transmission lines" (657),
Boolean: "electric power" +geomagnetic +fluctuations +amperes (225), "electric power" +geomagnetic +amperes (716), "electric noise" +"transmission lines" (240),
Boolean: ulf +"from electric" (1,350), ulf emissions from power (128,000), "ulf emissions" +electric +(grid OR grids) (29),
Boolean: "electric power" +"solar storms" (21,000), "electric power" +"solar storms" +voltages (487), "electric power" +"solar storms" +induction (358),
Boolean: electromagnetic +noise +"power grid" +solar (21,400), electromagnetic +noise +"power grid" +geomagnetic (1,100), electromagnetic +noise +"power grid" +khz (6,980),
Boolean: site:nerc.com +geomagnetic (59), "electric reliability" +geomagnetic (749), "electric reliability" +"solar storms" (82), "electric reliability" +monitoring +geomagnetic (439), "solar storms" +transients +electrical (317), geomagnetic +induction +voltages (3,320), geomagnetic +models +"electric power" (23,400),
Terms: geomagnetic storms (297,000), geomagnetic storm (294,000), geomagnetic variations (30,700), ulf emissions (1,170), geomagnetic storm effects (1,370), solar storm effects (587), magnetic storm effects (1,990),
Terms: solar storms (906,000), geomagnetic storms (296,000), space weather (6,620,000), type ii radio signature (4), type iii radio signature (6), type iii radio emissions (73), type ii radio emissions (480), qt noise (7,540),
The Human Impacts of Solar Storms and Space Weather
Terms: interplanetary radio emissions (62), interplanetary radio burst (67), interplanetary radio bursts (328), interplanetary medium (127,000), interplanetary magnetic field (265,000),
NASA - Stereo/Waves - 1/f emissions patterns over time
Terms: unified radio and plasma wave experiment (347), ulysses urap (3,500), urap radio (81), solar radio burst (39,600), solar radio bursts (31,300), type i burst (908), type i bursts (1,730),
Terms: thermal solar bursts (0), nonthermal solar bursts (0), thermal solar burst (0), nonthermal solar burst (0),
Terms: plasma oscillations (66,000), electron plasma frequency (29,900), quasi-thermal noise (771), plasma frequency receiver (289), radio astronomy receiver (1,510), plasma frequency (203,000), cavity modes (77,600),
Terms: type ii radio bursts (9,870), type iii radio bursts (9,730), type ii burst (13,300), type iii burst (5,220), type ii bursts (12,100), type iii bursts (15,100),
Ulysses URAP Home Page at NASA/GSFC - Solar/Interplanetary radio emissions - Type III bursts, Data Download, Instrument,
Low Radio Frequency Limit of Solar Type III Bursts
Green Bank Solar Spectrometer - Data
NOAA Space Weather Prediction Center - ftp -
Terms: advanced composition explorer (84,200), green bank solar spectrometer (2), solar spectrometer (2,430), microwave radio telescope (240), microwave radiotelescope (8), solar 2000 (85,500), solar irradiance (845,000),
Boolean: khz +"1/f" (590,000), "radio emissions" +"1/f" (1,020), "radio burst" +"1/f" (302), "radio burst" +khz (1,580), "radio emissions" +khz (23,700), "radio astronomy receiver" +urap (58),
Terms: geoeffectiveness (20,600), magnetic cloud (76,100), solar wind density (32,600), magnetic cloud events (937), magnetospheric reaction (21),
Terms: solar terrestrial relation observatory (54), solar terrestrial probes (35,500), sun earth connection coronal and heliospheric investigation (11,400), secchi (8,340,000), wind spacecraft (46,700),
Terms: sun earth connection (232,000), sun earth (2,430,000), solar terrestrial (1,520,000),
Terms: coronal mass ejections (737,000), solar wind (12,100,000), solar ejections (1,650),
Terms: the radio sun (8,350), radio jove (37,800), real time solar wind (52,500),
The Radio Sun - It is thus often the first object an amateur radio astronomer will turn their uhf or microwave antenna toward when testing. If you can't detect the Sun, you probably won't be able to detect anything with your uhf or microwave radiotelescope. The quite sun is a relatively stable signal source and can be used to make a rough calibration of your systems sensitivity.
List of TYPE II/III/IV bursts from WAVES/WIND satellite
Daily updated ACE data which you can compare to your radio observations
