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Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

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<strong>2001</strong>0023278 Lembaga Penerbangan dan Antariksa Nasional, HF Communications, Jakarta, Indonesia<br />

Applying Multiquadric Methods for Mapping Indonesian Ionosphere f(0)F2 Penerapan Metode Multiquadric Untuk<br />

Pemetaan f(0)F2 Ionosfer Indonesia<br />

Jiyo, Lembaga Penerbangan dan Antariksa Nasional, Indonesia; Warta LAPAN; October 2000; ISSN 0126-9754; <strong>Volume</strong> 2, No.<br />

4, pp. 154-158; In Malay-Indonesian; Copyright; Avail: Issuing Activity<br />

In this paper we discuss the Multiquadric method for regional mapping of f(0)F2. This method can be used to make a map<br />

for region with irregular observation. Mathematically, the mapping method is simple <strong>and</strong> easy to apply. Application of the method<br />

for mapping the ionospherics f(0)F2 over Indonesia shows that there is increasing of f(0)F2 in the morning <strong>and</strong> latitudinal variation.<br />

It is characteristic of equatorial anomaly.<br />

Author<br />

Indonesia; Ionospherics; Mapping<br />

<strong>2001</strong>0023540 Lembaga Penerbangan dan Antariksa Nasional, HF Communications, Jakarta, Indonesia<br />

Relations Between Zonal Winds in the Lower Atmosphere <strong>and</strong> Fmin Above Biak Hubungan Antara Angin Zonal Di Atmosfer<br />

Bawah Dan Fmin Di Atas Biak<br />

Mumen, T., Lembaga Penerbangan dan Antariksa Nasional, Indonesia; Sjarifuddin, M., Lembaga Penerbangan dan Antariksa<br />

Nasional, Indonesia; Djamaluddin, T., Lembaga Penerbangan dan Antariksa Nasional, Indonesia; Warta LAPAN; October 2000;<br />

ISSN 0126-9754; <strong>Volume</strong> 2, No. 4, pp. 131-136; In Malay-Indonesian; Copyright; Avail: Issuing Activity<br />

Ionospheric layer (upper atmosphere) has an important role as reflection of high frequency waves because it contains charged<br />

particle. Lower atmosphere winds can change distribution of charged particle in the ionosphere, resulting ionospheric minimum<br />

frequency change (one of high frequency wave absorption indicator). Using zonal wind <strong>and</strong> fmin data of Biak (01 deg 08 min <strong>39</strong><br />

sec S; 136 deg 02 min 46 sec E), it is found that time interval of 6 days between fmin enhancements <strong>and</strong> reversal of stratospheric<br />

zonal wind direction from westward to eastward over stratosphere (about 27 km high).<br />

Author<br />

Zonal Flow (Meteorology); Wind (Meteorology); Wind Direction<br />

<strong>2001</strong>002<strong>39</strong>23 <strong>Aerospace</strong> Corp., Technology Operations, El Segundo, CA USA<br />

The Plasma Mantle: Polar Satellite Observations<br />

Fennell, J. F.; Roeder, J. L.; Gr<strong>and</strong>e, M.; Perry, C.; Friedel, R.; Dec. 20, 1998; 12p; In English<br />

Contract(s)/Grant(s): F04701-93-C-0094<br />

Report No.(s): AD-A385553; TR-99(8570)-10; SMC-TR-00-40; No Copyright; Avail: CASI; A03, Hardcopy; A01, Microfiche<br />

Since launch in February 1996, the Polar satellite has made numerous traversals of the high-latitude dayside magnetosphere.<br />

These traversals have covered the high-altitude regions of the low-latitude boundary layer, cusp, cleft, mantle, <strong>and</strong> polar cap.<br />

Often, as the Polar satellite traverses the high-latitude dayside magnetosphere, it leaves the soft precipitation region of the cusp<br />

or cleft <strong>and</strong> enters into the mantle plasma. There, the angular distribution of 1 to 10 keV ions changes character from a convecting<br />

near-isotropic one to convecting predominantly perpendicular ions that are weakly upflowing. Sometimes the predominantly perpendicular<br />

fluxes of ions are observed throughout the cusp, cleft, <strong>and</strong> mantle. These ’trapped’ ion signatures are relatively common,<br />

<strong>and</strong> the energy of the trapped ions is generally is less than 10 keV. The energy of the most poleward trapped population<br />

generally decreases with increasing latitude as is expected for the mantle plasma. The angular distributions of the downward-going<br />

is less than 10 keV ions have large ’loss cones’, indicative of a relatively weak mirror geometry in the magnetic field at high altitudes.<br />

The mantle ion fluxes observed on Polar show much the same flows, distributions, <strong>and</strong> spatial characteristics as those<br />

observed on HEOS Rosenbauer et al., 1975. The composition of the ions at is greater than 1 keV/q is predominantly solar wind<br />

as expected.<br />

DTIC<br />

Earth Magnetosphere; Plasma Sheaths; <strong>Scientific</strong> Satellites; Satellite Observation; Plasmas (Physics)<br />

<strong>2001</strong>00240<strong>39</strong> Massachusetts Inst. of Tech., Dept. of Aeronautics <strong>and</strong> Astronautics, Cambridge, MA USA<br />

Near-Real Time Atmospheric Density Model Correction Using Space Catalog Data<br />

Granholm, George R., Massachusetts Inst. of Tech., USA; Nov. 02, 2000; 186p; In English<br />

Contract(s)/Grant(s): IR&D-00-2-837; Proj. 15080<br />

Report No.(s): AD-A384662; CSDL-T-1380; CY00437; No Copyright; Avail: CASI; A09, Hardcopy; A02, Microfiche<br />

Several theories have been presented in regard to creating a neutral density model that is corrected or calibrated in near-real<br />

time using data from space catalogs. These theories are usually limited to a small number of frequently tracked ’calibration satellites’<br />

about which information such as mass <strong>and</strong> cross-sectional area is known very accurately. This work, however, attempts to<br />

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