Matches in SemOpenAlex for { <https://semopenalex.org/work/W2080931887> ?p ?o ?g. }
- W2080931887 endingPage "2505" @default.
- W2080931887 startingPage "2495" @default.
- W2080931887 abstract "Impulsive Pi2 pulsations have long been recognized as one of the key signatures of magnetic activity during substorm periods due to their wide observable range both in latitudes and longitudes. It is well documented that there is usually more than one Pi2 wave burst associated with a substorm and only one of them corresponds to the onset of the substorm. This observational fact poses obstacles to determining substorm onsets with Pi2 signals. Although the Pi2 have become one of the most popular indicators for substorm onsets, the reliability of using the Pi2 in this fashion has not been seriously investigated. In this paper we address this question with a statistical approach by using ∼650 auroral substorm onsets identified with Polar ultraviolet images for a time interval from April 1996 to May 1997. A comparison of the low‐latitude Pi2 pulsation onsets from Kakioka ( L = 1.07) with the auroral breakups indicates that identifying substorm onset with the Pi2 alone is often ambiguous. Of a total of 119 isolated (defined as ∼10 min of quiet time preceding the onset) Pi2 bursts seen within ∼10 min from a magnetic positive bay, there were 65 events (∼55%) taking place within 3 min from breakups and 34 events (29%) indicating no sign of an auroral breakup within 10 min of the Pi2 burst. This result suggests that Pi2 may not be as a good indicator of the substorm onset as it was thought to be. Interestingly, it is always possible to associate Pi2 pulsations with some forms of auroral intensification. When compared to auroral breakups, Pi2 onsets are subject to a small delay of 1 – 3 min, with a peak around l min. Delays of Pi2 onsets are revealed to be a function of location relative to auroral breakup. This dependence is found to be consistent with the time of flight for a fast‐mode wave, in a plasmapause cavity mode model, propagating in the magnetosphere." @default.
- W2080931887 created "2016-06-24" @default.
- W2080931887 creator A5004281837 @default.
- W2080931887 creator A5012493161 @default.
- W2080931887 creator A5035558738 @default.
- W2080931887 creator A5037929275 @default.
- W2080931887 creator A5050013047 @default.
- W2080931887 creator A5066399283 @default.
- W2080931887 creator A5080653933 @default.
- W2080931887 creator A5083926853 @default.
- W2080931887 date "2000-02-01" @default.
- W2080931887 modified "2023-10-09" @default.
- W2080931887 title "Evaluation of low‐latitude Pi2 pulsations as indicators of substorm onset using Polar ultraviolet imagery" @default.
- W2080931887 cites W1966154398 @default.
- W2080931887 cites W1969615300 @default.
- W2080931887 cites W1975933077 @default.
- W2080931887 cites W1976262040 @default.
- W2080931887 cites W1977754384 @default.
- W2080931887 cites W1978873108 @default.
- W2080931887 cites W1985781151 @default.
- W2080931887 cites W1986885774 @default.
- W2080931887 cites W1987608980 @default.
- W2080931887 cites W1988900587 @default.
- W2080931887 cites W199392309 @default.
- W2080931887 cites W1996562643 @default.
- W2080931887 cites W1997921770 @default.
- W2080931887 cites W2001808349 @default.
- W2080931887 cites W2005907575 @default.
- W2080931887 cites W2010774225 @default.
- W2080931887 cites W2018285347 @default.
- W2080931887 cites W2018985351 @default.
- W2080931887 cites W2020140485 @default.
- W2080931887 cites W2020631520 @default.
- W2080931887 cites W2027076235 @default.
- W2080931887 cites W2030871161 @default.
- W2080931887 cites W2035717463 @default.
- W2080931887 cites W2038100229 @default.
- W2080931887 cites W2038538671 @default.
- W2080931887 cites W2040097103 @default.
- W2080931887 cites W2049874631 @default.
- W2080931887 cites W2052737070 @default.
- W2080931887 cites W2053664628 @default.
- W2080931887 cites W2054695950 @default.
- W2080931887 cites W2065957194 @default.
- W2080931887 cites W2085037851 @default.
- W2080931887 cites W2092191185 @default.
- W2080931887 cites W2118436133 @default.
- W2080931887 cites W2149931818 @default.
- W2080931887 cites W2160664728 @default.
- W2080931887 cites W2164703798 @default.
- W2080931887 cites W4252419441 @default.
- W2080931887 cites W4362209264 @default.
- W2080931887 doi "https://doi.org/10.1029/1999ja900416" @default.
- W2080931887 hasPublicationYear "2000" @default.
- W2080931887 type Work @default.
- W2080931887 sameAs 2080931887 @default.
- W2080931887 citedByCount "91" @default.
- W2080931887 countsByYear W20809318872012 @default.
- W2080931887 countsByYear W20809318872013 @default.
- W2080931887 countsByYear W20809318872014 @default.
- W2080931887 countsByYear W20809318872016 @default.
- W2080931887 countsByYear W20809318872017 @default.
- W2080931887 countsByYear W20809318872018 @default.
- W2080931887 countsByYear W20809318872020 @default.
- W2080931887 countsByYear W20809318872021 @default.
- W2080931887 countsByYear W20809318872022 @default.
- W2080931887 crossrefType "journal-article" @default.
- W2080931887 hasAuthorship W2080931887A5004281837 @default.
- W2080931887 hasAuthorship W2080931887A5012493161 @default.
- W2080931887 hasAuthorship W2080931887A5035558738 @default.
- W2080931887 hasAuthorship W2080931887A5037929275 @default.
- W2080931887 hasAuthorship W2080931887A5050013047 @default.
- W2080931887 hasAuthorship W2080931887A5066399283 @default.
- W2080931887 hasAuthorship W2080931887A5080653933 @default.
- W2080931887 hasAuthorship W2080931887A5083926853 @default.
- W2080931887 hasBestOaLocation W20809318871 @default.
- W2080931887 hasConcept C115260700 @default.
- W2080931887 hasConcept C116403925 @default.
- W2080931887 hasConcept C121332964 @default.
- W2080931887 hasConcept C122523270 @default.
- W2080931887 hasConcept C127313418 @default.
- W2080931887 hasConcept C1276947 @default.
- W2080931887 hasConcept C130443932 @default.
- W2080931887 hasConcept C13280743 @default.
- W2080931887 hasConcept C157899998 @default.
- W2080931887 hasConcept C2777871205 @default.
- W2080931887 hasConcept C29705727 @default.
- W2080931887 hasConcept C2991837008 @default.
- W2080931887 hasConcept C44870925 @default.
- W2080931887 hasConcept C57879066 @default.
- W2080931887 hasConcept C62520636 @default.
- W2080931887 hasConcept C8058405 @default.
- W2080931887 hasConceptScore W2080931887C115260700 @default.
- W2080931887 hasConceptScore W2080931887C116403925 @default.
- W2080931887 hasConceptScore W2080931887C121332964 @default.
- W2080931887 hasConceptScore W2080931887C122523270 @default.
- W2080931887 hasConceptScore W2080931887C127313418 @default.
- W2080931887 hasConceptScore W2080931887C1276947 @default.