Terms: Acceleration Motion (1600), variable acceleration (993), random acceleration (323),
Terms: random vibration (107000), random motion (131000), perturbation equation (418), stochastic equation (1730), stochastic equations (42600), stochastic delay (1510),
Terms: stochastic (7780000), stochastic climate (824), stochastic Navier Stokes (661), randomly-forced (508), stochastic economics (141), stochastic diffusion (1010),
Terms: quantum noise (64200), ergodic (540000), noise (115000000), brownian motion (742000), random acceleration (323), random velocity (2690), random motion (131000), random speeds (836),
Terms: brownian acceleration (1), microphonic noise (851), noise cancelation (5060), noise level (3460000), noise levels (2140000),
Terms: seismic noise (16500), white noise (2930000), white noise generator (59500), pink noise (330000), flicker noise (38100), 1/f noise (106000), Voss-McCartney (59), audio spectrum (255000), reverse time (747000),
Terms: background noise (2650000), ambient noise (887000), broadband Rayleigh waves (14), ambient seismic noise (305), ambient light (1380000), ambient sonar (20), microseisms (1540), microseism (1320),
Terms: power density (814000), watts per hertz (174), watts per nanometer (44), rf exposure (93100), watts/m2 (33100), watts/cm2 (1860), microwatt/cm2 (93), femto watt/cm2 (0),
Terms: VLF (701000), VHF (7380000), UHF (5960000), L-Band (389000), S-Band (353000), C-Band (1150000), X-band (525000), Ku-Band (885000), K-Band (165000), Ka-Band (373000), V-Band (96400), equivalent power density (156),
Terms: ActionScript (4320000), ECMAScript (509000),
Terms: solar constant (92000),
Solar Constant = 1368 watts/m2 = 0.1368 watts/cm2
Terms: magnetic pressure (40500), magnetic tension (2870), magnetic pump (3940), magnetic force (512000),
Terms: magnetic flux (711000), magnetic field strength (261000), magnetic energy density (1200),
Power Densities of Interest - Many useful radiation numbers and relations
Sound - Standard benchmark = 10-16 watts/cm2
USGS OF 2005-1077: An Assessment of Seismic Noise Levels for the Advanced National Seismic System Backbone Network and Selected Regional Broadband Stations
The Lorentz Force - Magnetic Pressure and Tension
MAGNETIC FORCE: 1 Star Drive by John Gard
Magnetic Force: Magnetic Force Density
Terms: permanent magnets (411000), permanent magnet (997000), permanent magnetic (115000), remanence (115000), magnetic energy density product (2), coercive field (7670), hard magnetic (20600), magnetic hardness (204), rare earth magnets (201000), magnetic induction (185000), self inductance (65400),
Self-inductance of a coaxial line
Terms: magnetometer (788000), magnetometers (338000), gauss meter (191000), gaussmeter (45400), hall effect (776000), hall sensor (71900),
Terms: proton precession (2560), proton precession magnetometer (1130), proton magnetometer (1750), differential proton magnetometer (18), magnetic field measurement (12700),
Boolean: calibration AND "magnetic field" (331000), "standing wave" AND "magnetic field" (48100), "magnetic permeability" AND (measuring OR measurement) (16600), "hall probes" AND usb (33),
Terms: transverse electromagnetic (7700), tem cells (1690), Field strength sensors calibration (6), magnetic field pictures (46), teslameters (1900), nmr magnetometers (316), fluxgate magnetometer (42500), magnetic field meters (1990),
Terms: hall probes (2230), Helmholtz coils (14300), anti-Helmholtz (228), triaxial Helmholtz (40), square Helmholtz (37),
NIST - Equations for the Magnetic Field Produced by One or More Rectangular Loops of Wire in the Same Plane
Field strength sensors calibration
Dan's Homegrown Proton Precession Magnetometer Page
diameter in the 70-100 mm range (signal-to-noise ratio improves with increased sensor diameter); coil length equal to inside diameter; coil depth 10 to 50 percent of inside diameter; two coils wound in opposite directions spaced about 40 percent of inside diameter apart to cancel induced noise. Wound to Vladimir's specifications, the sensors should yield a signal level of 0.28 microvolt with a S/N ratio of 100 or better, using the same polarization current. As far as polarization current goes, the more the better, short of burning out the coils: more current => stronger field => more protons aligned => stronger signal