TY - JOUR
T1 - An Intercomparison of VLF and Sounding Rocket Techniques for Measuring the Daytime D Region Ionosphere: Theoretical Implications
AU - Siskind, D.E.
AU - Zawdie, K.A.
AU - Sassi, Fabrizio
AU - Drob, D.
AU - Friedrich, Martin
PY - 2018
Y1 - 2018
N2 - We compare the two approaches that have been used to measure the lowermost ionosphere,the measurement of the propagation of very low frequency (VLF) radio waves and the in situ samplingby sounding rockets. We focus on the altitude, latitude, and zenith angle variation of the electron densityprofiles inferred from these two observational techniques as compared with a theoretical photochemicalmodel. Our results show that below 68–70 km, the VLF data and the model agree better with each otherthan with the sounding rocket profile. At the lowest altitudes, near 60 km, both the VLF data and the modelshow a greater electron density at higher latitudes, consistent with a cosmic ray flux that increases withlatitude, whereas the limited rocket data show a maximum at the tropics. Above 68–70 km, the VLF data andthe sounding rockets agree better and at tropical latitudes, the model fails to reproduce the observations.Specifically, the calculated electron density is lower than the data by up to a factor of 2. Possible reasonsfor the model deficit include underestimates of the solar Lyman alpha flux, the solar X-ray flux and themesospheric nitric oxide density. Once these three factors are mitigated, the model is in agreement with theobservations between 60 and 80 km.
AB - We compare the two approaches that have been used to measure the lowermost ionosphere,the measurement of the propagation of very low frequency (VLF) radio waves and the in situ samplingby sounding rockets. We focus on the altitude, latitude, and zenith angle variation of the electron densityprofiles inferred from these two observational techniques as compared with a theoretical photochemicalmodel. Our results show that below 68–70 km, the VLF data and the model agree better with each otherthan with the sounding rocket profile. At the lowest altitudes, near 60 km, both the VLF data and the modelshow a greater electron density at higher latitudes, consistent with a cosmic ray flux that increases withlatitude, whereas the limited rocket data show a maximum at the tropics. Above 68–70 km, the VLF data andthe sounding rockets agree better and at tropical latitudes, the model fails to reproduce the observations.Specifically, the calculated electron density is lower than the data by up to a factor of 2. Possible reasonsfor the model deficit include underestimates of the solar Lyman alpha flux, the solar X-ray flux and themesospheric nitric oxide density. Once these three factors are mitigated, the model is in agreement with theobservations between 60 and 80 km.
KW - ionosphere atmosphere
U2 - 10.1029/2018JA025807
DO - 10.1029/2018JA025807
M3 - Article
SN - 0148-0227
VL - 123
SP - 8688
EP - 8697
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 10
ER -