مورد إلكتروني
Persistence of Auroral Electron Flux Events from DMSP/F9 Electron Measurements
| العنوان: | Persistence of Auroral Electron Flux Events from DMSP/F9 Electron Measurements |
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| المصدر: | DTIC AND NTIS |
| بيانات النشر: | 1992-01-31 |
| تفاصيل مُضافة: | RADEX INC BEDFORD MA Bounar, K. H. McNeil, W. J. |
| نوع الوثيقة: | Electronic Resource |
| مستخلص: | The persistence of auroral electron activity is examined and correlated to the geomagnetic activity, which is measured by the Kp index. To study this correlation the superposed epoch analysis technique was implemented. Epoch zero is the time at which Kp values persisted above a specified threshold value for a specified duration. It was found that a high correlation between enhanced Kp and the number of bright arcs can be achieved for a limited time. The waiting time to increase the chance of observing bright auroral arcs after enhanced Kp values are observed should be between 3 to 6 hours. Further, the substantial increase in the number of observations of intense events as a result of enhanced Kp lingers a maximum of 36 to 48 hours. After this time period, this number drops to the average number of random observations. |
| مصطلحات الفهرس: | Atmospheric Physics, Geomagnetism, GEOMAGNETISM, AURORAE, ELECTRON FLUX, METEOROLOGICAL SATELLITES, DMSP(DEFENSE METEOROLOGICAL SATELLITE PROGRAM), PRECIPITATING ELECTRONS, GEOMAGNETIC KP INDEX, SUPERIMPOSED EPOCH ANALYSIS, PE62101F, WUPLS32185AC, Text |
| URL: | |
| الإتاحة: | Open access content. Open access content Approved for public release; distribution is unlimited. |
| ملاحظة: | text/html English |
| أرقام أخرى: | DTICE ADA251241 832017380 |
| المصدر المساهم: | From OAIster®, provided by the OCLC Cooperative. |
| رقم الأكسشن: | edsoai.ocn832017380 |
| قاعدة البيانات: | OAIster |
| الوصف غير متاح. |