COMMISSION G:
Ionospheric Radio and Propagation (November
2004 – October 2007)
Edited
by Takashi Maruyama
G1.
Ionospheric Irregularities
G1.1.
Equatorial Spread F and Plasma Bubble
Onset
conditions and the evolution of plasma bubbles were studied in a
multi-instrumental atmosphere observation program, CPEA (Coupling Processes in
the Equatorial Atmosphere) [Fukao, 2006], including FAI (field-aligned
irregularity) mode operation of the Equatorial Atmosphere Radar (EAR) at
Kototabang in Sumatra Island, Indonesia [Yokoyama et al., 2004a, 2005a; Patra
et al., 2005; Yokoyama and Fukao, 2006; Fukao et al., 2006; Ogawa et al.,
2006a; Otsuka et al., 2006a]. EAR observations of FAI were compared with the
plasma blobs detected by the ROCSAT-1 satellite [Yokoyama et al., 2007].
Ionospheric height variations were studied in connection with onset conditions
of plasma bubbles [Saito and Maruyama, 2006, 2007] by using the ionospheric
sounding data from the Southeast Asia Ionospheric Network (SEALION) [Maruyama
et al., 2007]. Passive remote soundings of plasma bubbles and the related
structure were conducted by receiving TV broadcasting signals at VHF from
Southeast Asia countries [Nakata et al., 2004, 2005] and by receiving HF radio
broadcasting signals from Australia [Maruyama and Kawamura, 2006]. A greatly
developed plasma bubble extending over middle Japan, with an equatorial height
of approximately 2500 km, was detected by a dense GPS receiver network over
Japan, GEONET (GPS Earth Observation Network), [Ma and Maruyama, 2006]. A
geomagnetically conjugate aspect of well-developed plasma bubbles was observed
by all-sky imagers located in
G1.2.
Sporadic E and Quasi-Periodic Echo
A
multi-instrumental observation campaign, SEEK-2 (Sporadic E Experiment over
Kyushu 2), for sporadic E study was conducted around
Generation
mechanisms responsible for E-region field-aligned irregularities and
quasi-periodic (QP) echoes involved with neutral atmospheric dynamic were
studied using VHF radars, all sky imagers, and other experiments [Ogawa et al.,
2006b; Saito et al., 2006, 2007; Patra et al., 2007; Otsuka et al., 2007], in
numerical simulations [Yokoyama et al., 2004b], and through theoretical
approaches [Tsunoda et al., 2004; Haldoupis et al., 2005]. Global and seasonal
distribution of sporadic E was depicted by applying an occultation technique to
radio propagation data from the GPS satellites to the CHAMP satellite
[Garcia-Fernandez and Tsuda, 2006]. A correlation between the sporadic metal
layers and the sporadic E layer was studied with simultaneous lidar and
ionosonde observations over Kototabang in
G2.
Ionospheric Disturbances
G2.1.
Ionospheric Storm
Ionospheric
disturbances caused by the prompt penetration of magnetospheric electric fields
during major magnetic storms were demonstrated. [Mannucci et al., 2005;
Tsurutani et al., 2006] and model calculations were compared with the
observations [Pavlov et al., 2006; Pavlov and Fukao, 2007; Tsurutani et al.,
2007]. Observations including magnetometer data from the Pacific sector were
used to study the equatorial ionospheric electric field during a geomagnetic
storm [Fejer et al., 2007]. GEONET and an ionosonde network along the Japanfs
meridian were used to study geomagnetic storm effects on the ionosphere
disturbances [Unnikrishnan et al., 2005; Kutiev et al., 2005, 2006, 2007;
Maruyama, 2006; Maruyama and Nakamura, 2007], while observations in the East
Asian and Brazilian sectors were compared for studying global characteristics
of ionospheric storms [Sahai et al., 2005; Abdu et al., 2007]. Responses of the
D-region electron density to geomagnetic storms were studied by analyzing tweek
atmospherics in the ELF/VLF bands [Ohya et al., 2006].
G2.2
Direct Effect of Energetic Radiations
Increases in
EUV and soft X-ray radiations associated with solar flares cause ionospheric
disturbances. Characteristics of the ionospheric response to solar flares were
studied from sudden increases in the total electron content (SITEC) [Tsugawa et
al., 2006b, 2007], rapid thermospheric responses observed by the CHAMP
satellite [Liu, H. et al., 2007b], and changes in the amplitude of VLF signals
with short and long propagation distances [Todoroki et al., 2007]. An
ionospheric disturbance caused by another energetic event, a cosmic gamma-ray
burst, was detected by a riometer and other instruments [Maeda et al., 2005].
G2.3.
Traveling Ionospheric Disturbances
Geomagnetic
conjugate characteristics of traveling ionospheric disturbances were studied
with simultaneous observations in Japan and Australia by using an all-sky
airglow imager network [Shiokawa et al., 2005a] and GPS receiver networks over
Japan (GEONET) and Australia [Tsugawa et al., 2006a]. Midlatitude ionospheric
irregularities over
G2.4.
Other Disturbances Associated with Magnetic Storm
Low-latitude
aurora events in the northern sky of
G3.
GPS Application to Ionosphere Study
Several new
techniques were developed for ionospheric application of GPS signals. A
technique for determination of GPS differential biases and an ionospheric
tomography based on the artificial neural network technique was developed [Ma
et al., 2005a, b]. A combined use of limb sounding data with that from
ground-based GPS receiver and ionosonde networks improved the accuracy of an ionospheric
tomography [Garcia-Fernandez et al., 2005]. For the purpose of space weather
monitoring, a near real-time estimation procedure of TEC was developed based on
the GEONET data service [Miyake, 2007]. An improvement of the accuracy of
vertical TEC estimates was discussed for the oblate earthfs gravitational
equipotential surface model [Hobigar et al., 2007].
G4.
Ionospheric Structure and Models
G4.1.
Ionospheric Structure
A far ultraviolet
(FUV) imager onboard the IMAGE satellite revealed nighttime zonal structure of
the low latitude ionosphere with the wave-number-4 feature [Sagawa et al.,
2005; England et al., 2006; Immel et al., 2006]. An electron density
discontinuity or additional layering of the low latitude F region, sometimes
referred to as the F3 layer in the bottomside or to as an ionospheric ledge in
the topside, were studied by using topside soundings by the EXOS-C and ISIS-2
satellites [Uemoto et al., 2004, 2006] and bottomside soundings from a
meridional ionosonde network over Southeast Asia [Uemoto et al., 2007]. Chaotic
behavior of ionospheric fluctuations was studied in various geophysical
conditions using GPS TEC data [Unnikrishnan et al., 2006a, b].
A D-region electron
density profile was obtained at a noon high-latitude by using an LF/MF radio
receiver and a DC probe onboard a sounding rocket [Ishisaka et al., 2005].
G4.2.
Ionospheric Models
Long-term
databases of incoherent scatter radars including the MU radar at
G5.
Coupling with Atmosphere/Lithosphere
G5.1.
Neutral Atmosphere-Ionosphere System
Airglow
measurements near the equator over Kototabang in Sumatra Island, Indonesia
revealed quasi-periodic southward moving waves in the thermosphere [Shiokawa et
al., 2006a] and northward propagating front-like structure aligned in the
east-west direction in the mesosphere [Shiokawa et al., 2006b]. Thermospheric
winds at midlatitudes observed by the MU radar at
G5.2.
Effect of Thunder Storm and Meteorological Phenomenon
Coordinated
optical and electromagnetic (VLF/ELF/VHF) measurements of sprites, optical
emissions in the mesosphere associated with thunderstorm activities, were
conducted [Adachi et al., 2005; Matsudo et al., 2007]. Electrical properties of
lightning discharges that play an essential role in the initiation and
development of sprites were investigated [Ohkubo et al., 2005]. The ISUAL payload, space-based measurement of sprites for the first time,
onboard the FORMOSAT-2 satellite was launched [Mende et al., 2005]. The
electron energy and electric field were estimated from the spectral data, and
kinetic processes involved with sprites were studied [Adachi et al., 2006]. It was
numerically demonstrated that the time scale of charge removal by lighting is
an essential parameter for the initiation of sprites [Hiraki and Fukunishi,
2006]. Numerical simulations were made to study the behavior of positive
charges causing sprite halos using a particle model combined with a
quasi-electrostatic model [Tong et al., 2005]. Midlatitude ionospheric Alfvén
resonator (IAR) excitation due to electromagnetic waves radiated from lightning
discharges was studied analytically and numerically [Surkov et al., 2005,
2006]. The intensity of the Schumann resonance, global electromagnetic
oscillations, has been monitored at
G5.3.
Earthquake Effect on the Ionosphere
Upper
atmospheric perturbations stimulated by the great Sumatra earthquake on 26
December 2004 were detected as changes in the ionospheric total electron
content by GPS receiver networks [Otsuka et al., 2006b; Heki et al., 2006; Liu,
J.-Y. et al., 2006] and as geomagnetic pulsations generated through the dynamo
action of an atmospheric pressure pulse [Iyemori et al., 2005]. The observed
TEC disturbances were numerically modeled [Shinagawa et al., 2007]. A similar
TEC disturbance generated by a volcano eruption in central
A precursor
of ionospheric perturbations to the
G6.
Polar Atmosphere-Ionosphere
The cosmic
radio noise absorption (CNA) was measured at
Among the
backscattering from ionospheric irregularities, distinctive polar mesosphere
summer echoes (PMSEs) were detected by the oblique incidence SuperDARN radars
in the
A sounding
rocket was launched from Andøya Rocket Range, Norway in the Dynamics and
Energetics of the Lower Thermosphere in Aurora (DELTA) campaign [Abe et al.,
2006a], being coordinated with ground-based instruments. Atmospheric parameters
were obtained along the rocket trajectory in a diffuse aurora; the electron
density was increased by the auroral precipitation [Wakabayashi and Ono, 2006];
the electron temperature was remarkably high at 106-114 km altitudes [Abe et
al., 2006b]; observed energy spectra of energetic electrons were compared with
auroral images taken from the ground [Ogasawara et al., 2006]; the rotational
temperature and the density of molecular nitrogen were measured and compared
with the MSIS empirical model [Kurihara et al., 2006]; the neutral and electron
temperatures measured by the DELTA rocket were compared with neutral/ion and
electron temperatures observed by the EISCAT UHF radar [Nozawa et al., 2006].
References
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H. and Y. Miyoshi [2006], gCharacteristics of the large-scale traveling
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Fukao, S. [2006], gCoupling
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Garcia-Fernandez,
M. and T. Tsuda [2006], gA global distribution of sporadic E events revealed by
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Garcia-Fernandez,
M., A. Saito, J. M. Juan, and T. Tsuda [2005], gThree-dimensional estimation of
electron density over Japan using the GEONET GPS network combined with SAC-C
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Haldoupis, C.,
T. Ogawa, K. Schlegel, J. A. Koehler, and T. Ono [2005], gIs there a plasma density gradient role on the
generation of short-scale Farley-Buneman waves?,h Ann. Geophys., Vol. 23, pp.3323-3337.
Hayakawa, M., K. Ohta, A. P.
Nickolaenko, and Y. Ando [2005], gAnomalous effect
in Schumann resonance phenomena observed in Japan, possibly associated with the
Chi-chi earthquake in Taiwan,h Ann. Geophys., Vol. 23, pp.1335-1346.
Heki,
K. [2006], gExplosion energy of the 2004 eruption of the Asama Volcano, central
Heki,
K., Y. Otsuka, N. Choosakul, N. Hemmakorn, T. Komolmis, and T. Maruyama [2006],
gDetection of ruptures of Andaman fault segments in the 2004 great Sumatra
earthquake with coseismic ionospheric disturbances,h J. Geophys. Res., Vol.
111, B09313, doi:10.1029/2005JB004202.
Hiraki,
Y. and H. Fukunishi [2006], gTheoretical criterion of charge moment change by
lightning for initiation of sprites,h J. Geophys. Res., Vol. 111, A11305, doi:10.1029/2006JA011729.
Hobiger,
T., T. Kondo, Y. Koyama, R. Ichikawa, and R. Weber [2007], gEffect of the
Earth's oblateness on the estimation of global vertical total electron content
maps,h Geophys. Res. Lett., Vol. 34, L11113, doi:10.1029/2007GL029792.
Horie, T., T. Yamauchi, M. Yoshida,
and M. Hayakawa [2007], gThe wave-like structures of ionospheric perturbation associated with
Sumatra earthquake of 26 December 2004, as revealed from VLF observation in
Japan of NWC signals,h J. Atmos. Solar-Terr. Phys., Vol. 69,
pp.1021-1028, doi:10.1016/j.jastp.2007.03.012.
Hosokawa, K., T. Ogawa,
A. S. Yukimatu, N. Sato, and T. Iyemori [2004], gStatistics of Antarctic
mesospheric echoes observed with the SuperDARN Syowa radar,h Geophys. Res. Lett.,
Vol. 31, L02106, doi:10.1029/2003GL018776.
Hosokawa, K., T. Ogawa,
N. F. Arnold, M. Lester, N. Sato, and A. S. Yukimatu [2005], gExtraction of
PMSE from SuperDARN data,h Geophys. Res. Lett., Vol. 32,
L12801, doi:10.1029/2005GL022788.
Hosokawa,
K., K. Shiokawa, Y. Otsuka, A. Nakajima, T. Ogawa, and J. D. Kelly [2006],
gEstimating drift velocity of polar cap patches with all-sky airglow imager at
Resolute Bay, Canada,h Geophys. Res. Lett., Vol. 33, L15111, doi:10.1029/2006GL026916.
Immel,
T. J., E. Sagawa, S. L. England, S. B. Henderson, M. E. Hagan, S. B. Mende, H.
U. Frey, C. M. Swenson, and L. J. Paxton [2006], gControl of equatorial ionospheric
morphology by atmospheric tides,h Geophys. Res. Lett., Vol. 33, L15108, doi:10.1029/2006GL026161.
Ishii, M., M. Kubota, M. Conde,
R. W. Smith, and M. Krynicki [2004], gVertical wind distribution in the polar
thermosphere during Horizontal E
Region Experiment (HEX) campaign,h J. Geophys. Res., Vol. 109, A12311, doi:10.1029/2004JA010657.
Ishisaka, K., T. Okada, J. Hawkins, S.
Murakami, T. Miyake, Y. Murayama, I. Nagano, and H. Matsumoto [2005],
gInvestigation of electron density profile in the lower ionosphere by SRP-4
rocket experiment,h Earth Planets
Space, Vol. 57, pp.879-884.
Iyemori,
T., M. Nose, D. Han, Y. Gao, M. Hashizume, N. Choosakul, H. Shinagawa, Y.
Tanaka, M. Utsugi, A. Saito, H. McCreadie, Y. Odagi, and F. Yang [2005],
gGeomagnetic pulsations caused by the Sumatra earthquake on December 26, 2004,h
Geophys. Res. Lett., Vol. 32, L20807, doi:10.1029/2005GL024083.
Kotake, N., Y. Otsuka, T. Tsugawa, T. Ogawa, and A. Saito
[2006], gClimatological study of GPS total electron content variations caused
by medium-scale traveling ionospheric disturbances,h J. Geophys.
Res., Vol. 111, A04306, doi:10.1029/2005JA011418.
Kotake, N., Y. Otsuka, T.
Tsugawa, T. Ogawa, and A. Saito [2007], gStatistical study of medium-scale
traveling ionospheric disturbances observed with the GPS networks in Southern
California,h Earth Planets Space, Vol. 59, pp.95-102.
Kurihara, J., T. Abe, K. -I. Oyama, E.
Griffin, M. Kosch, A. Aruliah, K. Kauristie, Y. Ogawa, S. Komada, and N.
Iwagami [2006], gObservations of the lower thermospheric neutral temperature
and density in the DELTA campaign,h Earth
Planets Space, Vol. 58, pp.1123-1130.
Kutiev, I., S.
Watanabe, Y. Otsuka, and A. Saito [2005],
gTotal electron content behavior over
Kutiev, I.., Y. Otsuka, A.
Saito, and S. Watanabe [2006], gGPS observations of post-storm TEC enhancements
at low latitudes,h Earth Planets
Space, Vol. 58, pp.1479-1486.
Kutiev, I., Y. Otsuka, A. Saito, and T. Tsugawa [2007],
gLow-latitude total electron content enhancement at low geomagnetic activity
observed over
Larsen, M. F.,
M. Yamamoto, S. Fukao, R. T. Tsunoda, and A. Saito [2005], gObservations of neutral winds, wind shears, and wave
structure during a sporadic-E/QP event,h Ann. Geophys., Vol. 23,
pp.2369-2375.
Lei, J., R. G. Roble,
Liu, H., H. Lühr, S.
Watanabe, W. Köhler, V. Henize, and P. Visser [2006], gZonal winds in the equatorial upper thermosphere: Decomposing the solar
flux, geomagnetic activity, and seasonal dependencies,h J. Geophys. Res., Vol.
111, A07307, doi:10.1029/2005JA011415.
Liu, H., H. Lühr, and
Liu,
H., H. Lühr, S. Watanabe, W. Köhler, and C. Manoj [2007b], gContrasting
behavior of the thermosphere and ionosphere in response to the 28 October 2003
solar flare,h J. Geophys. Res., Vol. 112, A07305, doi:10.1029/2007JA012313.
Liu, H., C. Stolle, S.
Watanabe, T. Abe, M. Rother, and D. L. Cooke [2007c], gEvaluation of the IRI model using CHAMP
observations in polar and equatorial regions,h Adv. Space Res., Vol. 39, pp.904-909, doi:10.1016/j.asr.2006.08.006.
Liu,
J. -Y., Y. -B. Tsai, K. -F. Ma, Y. -I. Chen, H. -F. Tsai, C. -H. Lin, M.
Kamogawa, and C. -P. Lee [2006], gIonospheric GPS total electron content (TEC)
disturbances triggered by the 26 December 2004 Indian Ocean tsunami,h J.
Geophys. Res., Vol. 111, A05303, doi:10.1029/2005JA011200.
Liu,
J. -Y., C. C. Hsiao, C. H. Liu, M. Yamamoto, S. Fukao, H. Y. Lue, and F. S. Kuo
[2007], gVertical group and phase velocities of ionospheric waves derived from
the MU radar,h Radio Sci., Vol. 42, RS4014, doi:10.1029/2005RS003435.
Ma, G. and T. Maruyama [2006], gA super bubble detected by
dense GPS network at East Asian longitudes,h Geophys.
Res. Lett., Vol. 33, L21103, doi:10.1029/2006GL027512.
Ma,
X. F., T. Maruyama, G. Ma, and T. Takeda [2005a], gDetermination of GPS
receiver differential biases by neural network parameter estimation method,h
Radio Sci., Vol. 40, RS1002, doi:10.1029/2004RS003072.
Ma, X. F., T. Maruyama, G. Ma, and T. Takeda [2005b],
gThree-dimensional ionospheric tomography using observation data of GPS ground
receivers and ionosonde by neural network,h J. Geophys.
Res., Vol. 110, A05308, doi:10.1029/2004JA010797.
Maeda,
K., I. Tomizawa, T. F. Shibata, N. Tokimasa, A. Saito, and T. Maruyama [2005],
gIonospheric effects of the cosmic gamma ray burst of 29 March 2003,h Geophys.
Res. Lett., Vol. 32, L18807, doi:10.1029/2005GL023525.
Maeda,
S., S. Nozawa, Y. Ogawa, and H. Fujiwara [2005], gComparative study of the
high-latitude E region ion and
neutral temperatures in the polar cap and the auroral region derived from the
EISCAT radar observations,h J. Geophys. Res., Vol. 110, A08301, doi:10.1029/2004JA010893.
Maekawa, S., T.
Horie, T. Yamauchi, T. Sawaya, M. Ishikawa, M. Hayakawa, and H. Sasaki [2006],
gA statistical study on the effect of earthquakes on
the ionosphere, based on the subionospheric LF propagation data in
Mannucci,
A. J., B. T. Tsurutani, B. A. Iijima, A. Komjathy, A. Saito, W. D. Gonzalez, F.
L. Guarnieri, J. U. Kozyra, and R. Skoug [2005], gDayside global ionospheric
response to the major interplanetary events of October 29–30, 2003 gHalloween
Stormsh,h Geophys. Res. Lett., Vol. 32, L12S02, doi:10.1029/2004GL021467.
Maruyama,
T. [2006], gExtreme enhancement in total electron content after sunset on 8 November
2004 and its connection with storm enhanced density,h Geophys. Res. Lett., Vol.
33, L20111, doi:10.1029/2006GL027367.
Maruyama, T.
and M. Kawamura [2006], gEquatorial
ionospheric disturbance observed through a transequatorial HF propagation
experiment,h Ann.
Geophys., Vol. 24, pp.1401-1409.
Maruyama,
T. and M. Nakamura [2007], gConditions for intense ionospheric storms expanding
to lower midlatitudes,h J. Geophys. Res., Vol. 112, A05310, doi:10.1029/2006JA012226.
Maruyama, T.,
Maruyama, T., M. Kawamura, S. Saito, K.
Nozaki, H. Kato, N. Hemmakorn, T. Boonchuk, T. Komolmis, and C. Ha Duyen
[2007], gLow latitude
ionosphere-thermosphere dynamics studies with inosonde chain in Southeast
Asia,h Ann.
Geophys., Vol. 25, pp.1569-1577.
Matsudo, Y., T. Suzuki, M.
Hayakawa, K. Yamashita, Y. Ando, K. Michimoto, and V. Korepanov [2007], gCharacteristics of Japanese winter sprites and
their parent lightning as estimated by VHF lightning and ELF transients,h J. Atmos. Solar-Terr. Phys., Vol. 69,
pp.1431-1446, doi:10.1016/j.jastp.2007.05.002.
Mende, S. B., H. U. Frey, R. R. Hsu, H. T. Su, A. B.
Chen, L. C. Lee, D. D. Sentman, Y. Takahashi, and H. Fukunishi [2005], gD
region ionization by lightning-induced electromagnetic pulses,h J. Geophys.
Res., Vol. 110, A11312, doi:10.1029/2005JA011064.
Miyake, W. [2007], gPrompt derivation of TEC from GEONET data for
space weather monitoring in
Nakata,
H., Y. Akaike, Y. Otsuka, T. Takano, S. Ujigawa, and I. Nagashima [2004],
gRay-tracing calculation of VHF radio waves scattered by field-aligned
irregularities associated with equatorial plasma bubbles,h IEEJ Trans. FM, Vol.
124, pp.1253-1254.
Nakata,
H., I. Nagashima, K. Sakata, Y. Otsuka, Y. Akaike, T. Takano, S. Shimakura, K.
Shiokawa, and T. Ogawa [2005], gObservations of equatorial plasma bubbles using
broadcast VHF radio waves,h Geophys. Res. Lett., Vol. 32, L17110, doi:10.1029/2005GL023243.
Nakazawa, Y., T. Okada,
and K. Shiokawa [2004], gUnderstanding the gSEKKIh phenomena in Japanese
historical literatures based on the modern science of low-latitude aurora,h
Earth Planets Space, Vol. 56, pp.e41-e44.
Nickolaenko, A. P.,
M. Hayakawa, M. Sekiguchi, Y. Ando, and K. Ohta [2006], gModel modifications in Schumann resonance intensity
caused by a localized ionosphere disturbance over the earthquake epicenter,h Ann. Geophys., Vol. 24,
pp.567-575.
Nickolaenko, A. P. and M. Hayakawa [2007], gRecent studies of
Schumann resonance and ELF transients,h J. Atmos. Electr., Vol. 27, pp.19-39.
Nishino,
M., K. Makita, K. Yumoto, Y. Miyoshi, N. J. Schuch, and M. A. Abdu [2006],
gEnergetic particle precipitation in the Brazilian geomagnetic anomaly during
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