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MAGDAS FM-CW observation network 10min resolution data at Manila, Philippines

ResourceID
spase://IUGONET/NumericalData/ICSWSE/MAGDAS-FMCW/MNL/fmcw/PT10M_ICSWSE_binary

Description
Vertical drift velocity (and virtual height) of ionospheric plasmas observed at MAGDAS Manila station, Philippines. The time resolution is 10 minutes.

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Version:2.5.0

NumericalData

ResourceID
spase://IUGONET/NumericalData/ICSWSE/MAGDAS-FMCW/MNL/fmcw/PT10M_ICSWSE_binary
ResourceHeader
ResourceName
MAGDAS FM-CW observation network 10min resolution data at Manila, Philippines
ReleaseDate
2013-01-03 00:00:00
ExpirationDate
2199-12-31 00:00:00
Description
Vertical drift velocity (and virtual height) of ionospheric plasmas observed at MAGDAS Manila station, Philippines. The time resolution is 10 minutes.
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://IUGONET/Person/Akimasa.Yoshikawa
2. MetadataContact spase://IUGONET/Person/Shuji.Abe

AccessInformation
RepositoryID
Availability
Online
AccessRights
Restricted
AccessURL
Format
Binary
Acknowledgement
Scientists who want to engage in collaboration with ICSWSE should contact the project leader of MAGDAS/CPMN observations, Dr. A. Yoshikawa, Kyushu Univ., who will organize such collaborations. There is a possibility that the PI of MAGDAS will arrange offers so that there is less overlapping of themes between MAGDAS research groups. Before you use MAGDAS/CPMN data for your papers, you must agree to the following points; 1. Before you submit your paper, you must contact the PI and discuss authorship. 2. When you submit your paper after doing the above item 1, you must mention the source of the data in the acknowledgment section of your paper. 3. In general, you must use the following references: (i). Yumoto, K., and the 210MM Magnetic Observation Group, The STEP 210 magnetic meridian network project, J. Geomag. Geoelectr., 48, 1297-1310., 1996. (ii). Yumoto, K. and the CPMN Group, Characteristics of Pi 2 magnetic pulsations observed at the CPMN stations: A review of the STEP results, Earth Planets Space, 53, 981-992, 2001. (iii). Yumoto K. and the MAGDAS Group, MAGDAS project and its application for space weather, Solar Influence on the Heliosphere and Earth's Environment: Recent Progress and Prospects, Edited by N. Gopalswamy and A. Bhattacharyya, ISBN-81-87099-40-2, pp. 309-405, 2006. (iv). Yumoto K. and the MAGDAS Group, Space weather activities at SERC for IHY: MAGDAS, Bull. Astr. Soc. India, 35, pp. 511-522, 2007. 4. In all circumstances, if anything is published you must send a hardcopy to the following address: Dr. Akimasa Yoshikawa, PI of MAGDAS/CPMN Project, International Center for Space Weather Science and Education, Kyushu University 53, 6-10-1 Hakozaki, Higashi-ku Fukuoka 812-8581, JAPAN, TEL/FAX:+81-92-642-4403, e-mail: yoshi@geo.kyushu-u.ac.jp
ProcessingLevel
Calibrated
InstrumentIDs
MeasurementType
Profile
TemporalDescription
TimeSpan
StartDate
2009-03-19 00:00:00
RelativeStopDate
P1D
Cadence
PT10M
ObservedRegion
Earth.NearSurface.Ionosphere.ERegion
SpatialCoverage
CoordinateSystem
CoordinateRepresentation
Spherical
CoordinateSystemName
GEO
NorthernmostLatitude
14.63
SouthernmostLatitude
14.63
EasternmostLongitude
121.08
WesternmostLongitude
121.08
Keywords
Ionosphere plasma velosity virtual height radar
Parameter #1
Name
Drift velocity
Description
Vertical drift velocity of ionospheric E-layer plasmas.
Units
m/s
FillValue
-9999.0
Support
SupportQuantity
Velocity