|
|
| |
 | MAGDAS observation network 1sec resolution geomagnetic field data at Tirunelveli, India
 |
| |
|
|
| Timespan [day(s)]: 1, 3, 7 |
 |
| |
| Description: |
| Geomagnetic field data observed at MAGDAS Tirunelveli station, India. The time resolution is 1 second. The data consist of 3 components (H, D, Z) and total geomagnetic field (F) value. |
| ReleaseDate: 2013-07-30T00:00:00 |
| |
|
Contact
(PrincipalInvestigator):
|
| Akimasa Yoshikawa, International Research Center for Space and Planetary Environmental Science(i-SPES), Kyushu University, yoshikawa.akimasa.254@m.kyushu-u.ac.jp |
|
Contact
(MetadataContact):
|
| Shuji Abe, International Research Center for Space and Planetary Environmental Science(i-SPES), Kyushu University, abeshu@i-spes.kyushu-u.ac.jp |
| |
| AccessInformation: |
|
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 (Dr. A. Yoshikawa: yoshi@geo.kyushu-u.ac.jp) 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, 744, Motooka, Nishi-ku, Fukuoka, 819-0395, JAPAN, TEL/FAX:+81-92-802-6240, e-mail: yoshi@geo.kyushu-u.ac.jp |
|
URL: http://data.icswse.kyushu-u.ac.jp/ |
|
Availability: Online |
|
Access
Rights: Restricted |
|
Format: Binary |
| |
| Processing
Level: Calibrated |
| Measurement
Type: Magnetogram |
| |
| Time
Span: |
|
StartDate: 2007-09-28T00:00:00 |
| StopDate: P1D |
| |
| Observed
Region: Earth.Magnetosphere |
| |
| Keywords: ground observation magnetometer geomagnetic field |
| |
| Instrument: |
| Name: MAGDAS fluxgate magnetometer at TIR |
| Description: 3-axis ring-core type fluxgate magnetometer installed at Tirunelveli, India |
|
Contact
(PrincipalInvestigator):
|
| Akimasa Yoshikawa, International Research Center for Space and Planetary Environmental Science(i-SPES), Kyushu University, yoshikawa.akimasa.254@m.kyushu-u.ac.jp |
|
Contact
(MetadataContact):
|
| Shuji Abe, International Research Center for Space and Planetary Environmental Science(i-SPES), Kyushu University, abeshu@i-spes.kyushu-u.ac.jp |
| InstrumentType: Magnetometer |
| InvestigationName: MAGDAS observation network |
| |
| Observatory: |
| Name: MAGDAS Tirunelveli station |
| Description: MAGDAS magnetometer network, Tirunelveli, India |
|
Contact
(PrincipalInvestigator):
|
| Akimasa Yoshikawa, International Research Center for Space and Planetary Environmental Science(i-SPES), Kyushu University, yoshikawa.akimasa.254@m.kyushu-u.ac.jp |
|
Contact
(MetadataContact):
|
| Shuji Abe, International Research Center for Space and Planetary Environmental Science(i-SPES), Kyushu University, abeshu@i-spes.kyushu-u.ac.jp |
| Location: |
| ObservatoryRegion: Earth.Surface |
| CoordinateSystemName: GEO |
| Latitude: 8.7 |
| Longitude: 77.8 |
|
|
Observed
Data:
|
|
|
How to Plot (SPEDAS-CUI):
IDL>
THEMIS>
THEMIS>
THEMIS>
thm_init
timespan, ['2025-05-06 00:00:00', '2025-05-13 00:00:00']
iug_load_gmag_magdas_1sec, site='tir', datatype='1sec'
tplot, 'magdas_mag_tir_1sec_hdz'
|
|
How to Plot (SPEDAS-GUI [*Quick-Look was created with this command]):
IDL>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
thm_init
timespan, ['2025-05-06 00:00:00', '2025-05-13 00:00:00']
iug_load_gmag_magdas_1sec, site='tir', datatype='1sec'
tdpwrspc, 'magdas_mag_tir_1sec_hdz', nboxpoints=512, nshiftpoints=256
zlim, 'magdas_mag_tir_1sec_hdz_x_dpwrspc', 1e-4, 1e+3
zlim, 'magdas_mag_tir_1sec_hdz_y_dpwrspc', 1e-4, 1e+3
zlim, 'magdas_mag_tir_1sec_hdz_z_dpwrspc', 1e-4, 1e+3
options, 'magdas_mag_tir_1sec_hdz_x', 'ytitle', 'TIR!CH-comp'
options, 'magdas_mag_tir_1sec_hdz_y', 'ytitle', 'TIR!CD-comp'
options, 'magdas_mag_tir_1sec_hdz_z', 'ytitle', 'TIR!CZ-comp'
options, 'magdas_mag_tir_1sec_hdz_x', 'ysubtitle', '[nT]'
options, 'magdas_mag_tir_1sec_hdz_y', 'ysubtitle', '[nT]'
options, 'magdas_mag_tir_1sec_hdz_z', 'ysubtitle', '[nT]'
options, 'magdas_mag_tir_1sec_hdz_x_dpwrspc', 'ytitle', 'TIR!CPSD(H)!CFrequency'
options, 'magdas_mag_tir_1sec_hdz_y_dpwrspc', 'ytitle', 'TIR!CPSD(D)!CFrequency'
options, 'magdas_mag_tir_1sec_hdz_z_dpwrspc', 'ytitle', 'TIR!CPSD(Z)!CFrequency'
options, 'magdas_mag_tir_1sec_hdz_x_dpwrspc', 'ysubtitle', '[Hz]'
options, 'magdas_mag_tir_1sec_hdz_y_dpwrspc', 'ysubtitle', '[Hz]'
options, 'magdas_mag_tir_1sec_hdz_z_dpwrspc', 'ysubtitle', '[Hz]'
tplot_options, 'region', [0.05, 0, 1, 1]
tplot, ['magdas_mag_tir_1sec_hdz_x', 'magdas_mag_tir_1sec_hdz_y', 'magdas_mag_tir_1sec_hdz_z', 'magdas_mag_tir_1sec_hdz_x_dpwrspc', 'magdas_mag_tir_1sec_hdz_y_dpwrspc', 'magdas_mag_tir_1sec_hdz_z_dpwrspc']
|
|
How to Plot (UDAS Latest Version #Basic):
Note: UDAS latest versoin has not been included in SPEDAS yet, please download that from IUGONET web site. http://www.iugonet.org/product/analysis.jsp
IDL>
THEMIS>
THEMIS>
THEMIS>
thm_init
timespan, ['2025-05-06 00:00:00', '2025-05-13 00:00:00']
iug_load_gmag_icswse_iaga, site='tir', resolution='1sec'
tplot, ['kyumag_mag_tir_1sec_hdzf']
|
|
How to Plot (UDAS Latest Version #Advanced [*Quick-Look was created with this command]):
Note: UDAS latest versoin has not been included in SPEDAS yet, please download that from IUGONET web site. http://www.iugonet.org/product/analysis.jsp
IDL>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
THEMIS>
thm_init
timespan, ['2025-05-06 00:00:00', '2025-05-13 00:00:00']
iug_load_gmag_icswse_iaga, site='tir', resolution='1sec'
tdpwrspc, 'kyumag_mag_tir_1sec_hdzf', nboxpoints=512, nshiftpoints=256
zlim, 'kyumag_mag_tir_1sec_hdzf_0_dpwrspc', 1e-4, 1e+3
zlim, 'kyumag_mag_tir_1sec_hdzf_1_dpwrspc', 1e-4, 1e+3
zlim, 'kyumag_mag_tir_1sec_hdzf_2_dpwrspc', 1e-4, 1e+3
options, 'kyumag_mag_tir_1sec_hdzf_0', 'ytitle', 'TIR!CH-comp'
options, 'kyumag_mag_tir_1sec_hdzf_1', 'ytitle', 'TIR!CD-comp'
options, 'kyumag_mag_tir_1sec_hdzf_2', 'ytitle', 'TIR!CZ-comp'
options, 'kyumag_mag_tir_1sec_hdzf_0', 'ysubtitle', '[nT]'
options, 'kyumag_mag_tir_1sec_hdzf_1', 'ysubtitle', '[nT]'
options, 'kyumag_mag_tir_1sec_hdzf_2', 'ysubtitle', '[nT]'
options, 'kyumag_mag_tir_1sec_hdzf_0_dpwrspc', 'ytitle', 'TIR!CPSD(H)!CFrequency'
options, 'kyumag_mag_tir_1sec_hdzf_1_dpwrspc', 'ytitle', 'TIR!CPSD(D)!CFrequency'
options, 'kyumag_mag_tir_1sec_hdzf_2_dpwrspc', 'ytitle', 'TIR!CPSD(Z)!CFrequency'
options, 'kyumag_mag_tir_1sec_hdzf_0_dpwrspc', 'ysubtitle', '[Hz]'
options, 'kyumag_mag_tir_1sec_hdzf_1_dpwrspc', 'ysubtitle', '[Hz]'
options, 'kyumag_mag_tir_1sec_hdzf_2_dpwrspc', 'ysubtitle', '[Hz]'
tplot_options, 'region', [0.05, 0, 1, 1]
tplot, ['kyumag_mag_tir_1sec_hdzf_0', 'kyumag_mag_tir_1sec_hdzf_1', 'kyumag_mag_tir_1sec_hdzf_2', 'kyumag_mag_tir_1sec_hdzf_0_dpwrspc', 'kyumag_mag_tir_1sec_hdzf_1_dpwrspc', 'kyumag_mag_tir_1sec_hdzf_2_dpwrspc']
|
|
How to Plot (SPEDAS-GUI Next Version):
Note: This operation is for SPEDAS released soon. See SPEDAS web site. http://spedas.org/
Step 1:
Step 2:
Step 3:
Step 4:
Step 5:
Step 6:
Step 7:
Step 8:
Step 9:
Step 10:
Step 11:
Step 12:
Start SPEDAS GUI Program.
Choose [FILE] -> [Load Data].
Choose [IUGONET] Tab.
Uncheck 'Use Single Day'.
Set Start Time: '2025-05-06 00:00:00' and Stop Time: '2025-05-13 00:00:00'.
Choose Instrument Type: 'geomagnetic_field_fluxgate'.
Choose Data Type: 'icswse', Site or parameter(s)-1: 'tir' and parameter(s)-2: '1sec'.
Push [->] button. (Please wait a few minutes).
Push [Done] button.
Choose [Graph] -> [Plot Layout Options].
Choose 'kyumag_mag_tir_1sec_hdzf' and push [Line->] button.
Push [OK] button.
|
|
Original
Metadata Files:
PT1S_ICSWSE_storage.xml:
MAGDAS observation network 1sec resolution geomagnetic field data at Tirunelveli, India
(Observatory)
TIR.xml:
MAGDAS Tirunelveli station
(Instrument)
fluxgate.xml:
MAGDAS fluxgate magnetometer at TIR
(Person)
Akimasa.Yoshikawa.xml:
Akimasa Yoshikawa
(Person)
Shuji.Abe.xml:
Shuji Abe
|
| |
|
|
