로그인 하지 않고 손님이 뉴스 홈을 이용할 경우, 메뉴가 자동으로 순환되면서 고정되지 않는 문제로 불편하실 수 있습니다. 가능하면 로그인 하시기 바랍니다.

Realtime Monitor Page (NEW)

이 글에 점수주기

Global or composite earthquake information, research or special services
지진관측 네트워크 정보
http://www.geophys.washington.edu/seismosurfing.html

GEOFON Extended Virtual Network - GEVN
http://geofon.gfz-potsdam.de/geofon/new/netabs/eq_inf_nets.html

유럽 지중해 지진센터(EMSC)
http://www.emsc-csem.org/index.php?page=home
http://www.emsc-csem.org/index.php?page=current⊂=map&map=world (Map Animation)

스위스 기록계
http://www.orfeus-eu.org/Earthquakes/recentquakes.html
http://www.orfeus-eu.org/Earthquakes/recentquakes_googlemaps.html
http://www.orfeus-eu.org/Earthquakes/europe.html
http://www.orfeus-eu.org/Earthquakes/world.htm

이탈리아 기록계
http://mednet.rm.ingv.it/earthquakes.php

독일 기록계 GEOFON
http://geofon.gfz-potsdam.de/db/eqinfo.php
http://geofon.gfz-potsdam.de/geofon//seismon/globmon.html

그리스 기록계
http://bbnet.gein.noa.gr/alerts_manual/maps/maps48h.html

중국 기록계
http://www.csndmc.ac.cn/newweb/index.jsp
http://www.csndmc.ac.cn/newweb/data/csn_fast_p002.jsp

ASEAN Earthquakes Information Center
http://aeic.bmg.go.id/mapperaeic.asp

Station의 모니터링 Plot;
http://www.wavero.net/forum/showthread.php?t=1545&page=4
http://aslwww.cr.usgs.gov/Seismic_Data/heli2.shtml

여기는 지진 모니터 3입니다.

지구자기장 시물레이션 그래프 해설
http://www.wavero.net/forum/content/1872-지구-자기장-시물레이션-그래프를-통한-자기장-변화의-해석

ACE의 자기장 변화곡선입니다.

Dynamic ACE RTSW Plots

Dur	SOLAR WIND:Mag field & Plasma	Magnetic Field	Plasma	Low Energy Electrons & Protons	Low Energy Electrons	Low Energy Protons	High Energy Protons
2 hrs	MAG_SWEPAM	MAG	SWEPAM	EPAM	EPAMe	EPAMp	SIS
6 hrs	MAG_SWEPAM	MAG	SWEPAM	EPAM	EPAMe	EPAMp	SIS
24 hrs	MAG_SWEPAM	MAG	SWEPAM	EPAM	EPAMe	EPAMp	SIS
3 days	MAG_SWEPAM	MAG	SWEPAM	EPAM	EPAMe	EPAMp	SIS
7 days	MAG_SWEPAM	MAG	SWEPAM	EPAM	EPAMe	EPAMp	SIS

Geomagnetic K-indices

This chart is updated every 15 minutes at 1, 16, 31, and 46 minutes past the hour. Use the browser Refresh or Reload option to ensure the latest data is shown. Boulder, Colorado and Fredericksburg, Virginia are mid-latitude stations. College, Alaska is a high-latitude station. Estimated Planetary is a combined measure of several mid- and high-latitude stations.
K-index Warnings are issued when a Boulder K-indices of 4, 5, 6, and 7 or greater is expected.
K-index Alerts are issued when the Boulder K-index reaches 4, 5, 6, 7, 8, or 9 in a 3-hour period.
NOAA Boulder Magnetometer
http://www.swpc.noaa.gov/rt_plots/bou_12h.html

Geomagnetic A-indices

This chart is updated every 15 minutes at 1, 16, 31, and 46 minutes past the hour. Use the browser Refresh or Reload option to ensure the latest data is shown. Boulder, Colorado and Fredericksburg, Virginia are mid-latitude stations. College, Alaska is a high-latitude station. Estimated Planetary is a combined measure of several mid- and high-latitude stations.
A-index Watches are issued when a Fredericksburg, Virginia (mid-latitude) A-index of greater than 20, 30, 50, or 100 is predicted. These thresholds are marked on the chart. When observed A-indices exceed 100, the charts are individually scaled as needed.

태양의 코로나 활동에 따른 양성자Proton의 증가, 자기에너지장의 변화등을 한눈에 보시려면, http://www.lmsal.com/solarsoft/last_events/ 를 참조하시기 바랍니다.

실시간이므로 점차 바뀌겠지만, http://www2.nict.go.jp/y/y223/simulation/realtime/ 에서 지속적인 변화를 보실 수 있습니다. 아래 그림은, 프라즈마 온도와 밀도, 정지궤도에서의 AE 인덱스 그래프입니다.

ACE의 자기장 변화곡선입니다.

HAARP Magnetometer, 1 Week, 하프 자기계 데이타

HAARP Magnetometer, 1 Month, 하프 자기계 데이타

참고, 2010년 5월 3일 자료

HAARP Induction Magnetometer, 하프 전도 자기계 X,Y,Z

HAARP의 주파수 결과는, http://www.haarp.alaska.edu/haarp/data.html
http://137.229.36.30/cgi-bin/magnetometer/gak-mag.cgi

The chart below is a plot of the readings taken using the HAARP VHF Riometer. This instrument is a sensitive receiver tuned to a frequency of 30 MHz. The antenna is an array of 4 element "yagi" type elements pointed directly upward to listen to the background or galactic noise. This noise varies from one hour to the next as the Earth rotates and, in the absence of ionospheric absorption, is a constant, repeatable function of Local Siderial Time. Over many observations, it is possible to develop a "quiet day" curve which represents the greatest noise that would be heard for any given hour of the day. By comparing the current noise measurement with the quiet day level, the current 30 MHz ionospheric absorption level can be derived and this number is shown in the figure. Solar-terrestrial events, such as geomagnetic storms are usually indicated by increases in the absorption level. The absorption at lower frequencies in the HF band is usually much higher than the level observed at 30 MHz. Occasional spikes in the received signal that go above the quiet day curve are caused by interference from broadcast signals in the 30 MHz band. Click here for a larger plot without this text.
HAARP 신호감지(검파)

GOES 의 X-Ray chart입니다. 파장이 짧아 에너지가 2배 더 강한 파란색 선과, 파장의 길이가 2배 긴 빨간선.

플라즈마, 양성자(포톤), 전자 모니터링입니다.

인용한 그래프는 SOHO 위성으로부터 받은 양성자 증감에 관한 그래프입니다. 양성자가 대기층에 증가한 경우는 태양으로부터의 유입을 들 수 있을텐데, 많은 양성자가 생기면 이에 반하여 전자Electron의 소모 또한 뒤따르게 될 것입니다. 전자가 양성자와 결합하는 양이 증가하면, 전자가 방출하는 광자Photon 역시 늘어나면서 더 많은 정보와 빛을 전달하는 과정이 될 것입니다.
실시간이므로 점차 바뀌겠지만, http://www2.nict.go.jp/y/y223/simulation/realtime/ 에서 지속적인 변화를 보실 수 있습니다. 아래 그림은, 프라즈마 온도와 밀도, 정지궤도에서의 AE 인덱스 그래프입니다.

스테레오 관련사이트

STEREO consists of two space-based observatories - one ahead of Earth in its orbit, the other trailing behind. With this new pair of viewpoints, scientists will be able to see the structure and evolution of solar storms as they blast from the Sun and move out through space.

http://stereo.gsfc.nasa.gov/
http://stereo-ssc.nascom.nasa.gov/beacon/beacon_secchi.shtml
http://stereo-ssc.nascom.nasa.gov/browse/

스테레오/SOHO 관련사이트, First tab content.


Latest EUVI Images This movie shows a spherical map of the Sun as it currently appears, formed from a combination of the latest STEREO Ahead and Behind beacon images. The movie starts with the view of the Sun as seen from Earth, with the 0 degree meridian line in the middle. The map then rotates through 360 degrees to show the part of the Sun not visible from Earth. The black wedge shows the part of the Sun not yet visible to the STEREO spacecraft. The images above are shown in the order of the relative positions of the three viewpoints, Behind, Earth, and Ahead. For the Heliospheric Imager (HI) images below, the order is reversed to reflect the fact that the HI Ahead telescopes look to the left of the Sun, and those on Behind look to the right. Also, the HI images are not rotated to put solar north up.
Helio Graphic
STEREO POSITION http://stereo-ssc.nascom.nasa.gov/where.shtml This figure plots the current positions of the STEREO Ahead (red) and Behind (blue) spacecraft relative to the Sun (yellow) and Earth (green). The dotted lines show the angular displacement from the Sun. Units are in A.U. When the two spacecraft are close to Earth, an expanded view of the region around Earth will appear on the right, in the same orientation as the Sun-centered view.