Observations and Analysis of Interplanetary Scintillation |
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Page 27
... values of the Table are left in terms relative to CTA - 21 at 430 MHz , for easier comparison with previously ... second moment of the power spectrum . In certain cases , an abnormally high square - root second moment was observed far ...
... values of the Table are left in terms relative to CTA - 21 at 430 MHz , for easier comparison with previously ... second moment of the power spectrum . In certain cases , an abnormally high square - root second moment was observed far ...
Page 57
... value of μ is quite low . This undoubtedly is affecting the second moment values somewhat , but the values are extremely low . source is certain to have several components however , as the value of μ after correction for finite angular ...
... value of μ is quite low . This undoubtedly is affecting the second moment values somewhat , but the values are extremely low . source is certain to have several components however , as the value of μ after correction for finite angular ...
Page 59
... second - moment position angle dependence . The values of the second - moment from 161-213 ° are quite high , almost identical to those of СТА - 21 . The four values observed at position angles 251 ° - 262 ° are quite low . Hewish and ...
... second - moment position angle dependence . The values of the second - moment from 161-213 ° are quite high , almost identical to those of СТА - 21 . The four values observed at position angles 251 ° - 262 ° are quite low . Hewish and ...
Contents
EXAMINATION OF SCINTILLATION BEHAVIOR | 10 |
FLUCTUATION SPECTRA AND SOURCE STRUCTURE | 78 |
INTERPLANETARY SCINTILLATION OF PULSARS | 127 |
2 other sections not shown
Common terms and phrases
angular diameter angular structure Ap.J arc sec Arecibo calculated Cohen complex source CORNELL CORNELL CORNELL LIBRARY Cornell University curve Ekers Elongation Modulation index equation F₂ Hz factor flare fluctuation power flux at 430 frequency proportional frequency spectrum function of frequency function of solar Gaussian Hewish index and square-root indicate intensity fluctuations interplanetary medium interplanetary scintillations interstellar medium interstellar scattering Jauncey km/sec LIBRARY CORNELL Lovelace lunar occultation measured meter wavelengths Nyquist frequency observations point source position angle Power spectrum power-law pulsar pulse radiation radio frequency radio sources Relative power density resolved Salpeter samples scale scattering angle scin screen second-moment values signal/noise Sine of Solar Solar Elongation Figure Solar Elongation Modulation solar wind velocity spectra square-root second square-root second moment strong scintillation regime tillation tion tiplied UNIVERSITY CORNELL value of µ VLBI VLBI data VLBI results wavenumber spectrum weak scintillation regime