Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Bloomfield, Shaun"'
Large and magnetically complex sunspot groups are known to be associated with flares. To date, the Mount Wilson scheme has been used to classify sunspot groups based on their morphological and magnetic properties. The most flare-prolific class, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::ff434477a8a67b5a731f41e509b6df86
My presentation I gave at ESWW13 explaining most recent work on sunspot group evolution and it's application as an operational forecasting tool
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2acdd7f2a9fbcb6d53084683b43de066
Poster presented at European Solar Physics Meeting, Trinity College Dublin, 2014 September 8 - 12 Trinity College Dublin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f0d57ade1d729714a113a4397b07b47
Poster presented at the "UK National Astronomy Meeting 2013" conference, 1st - 5th July 2013, St. Andrews, Scotland.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ace95b6e9ce9fe0512843b9500eb5a06
Poster presented at NAM 2013 in St. Andrews presenting the Coronal Pulse Identification and Tracking Algorithm (CorPITA) and showing how it identifies and analyses both an example of a wave and non-wave event.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d9e12404f728de72a5fca163a868b2d
Poster presented at the "UK National Astronomy Meeting 2013" conference, 1st - 5th July 2013, St. Andrews, Scotland.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::057cdc738e07555eb258b43e58ba9846
Autor:
O'Callaghan, David, Gallagher, Peter, Bloomfield, Shaun, Higgins, Paul, Pérez-Suárez, David, Murray, Sophie, Pierantoni, Gabriele, Roche, Joseph
Poster presented at the "UK National Astronomy Meeting 2013" conference, 1st - 5th July 2013, St. Andrews, Scotland. It is not currently possible to forecast solar flare occurrence to a high degree of accuracy. One of the best predictors for the occu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0db8d0d8558cb9c8592cc2fae26ee76a
This poster was presented at the American Geophysical Union 2013 Fall Meeting.The aim of this work is to determine statistically how important the 'sympathetic eruption' effect is. In conclusion, it is a weak effect overall: the occurrence of individ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b750fee58517ae58fe1f51ee93f37bc
We present an investigation of the large-scale flows that influence magnetic fields at the solar surface. The aim of this work is to accurately characterise the supergranular diffusion coefficient, D, that governs the dispersal rate of magnetic featu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::905f976db98074f00b4ebaf963e19536
Presentation at the plenary session of the Community of European Solar Radio Astronomers (CESRA) Workshop 2013 in Prague, given by Pietro Zucca on formation heights of coronal shock waves in the solar atmosphere.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70445b625f1ececf7a4e89a950bdb99d