Hasil Pencarian  ::  Simpan CSV :: Kembali

"Geomagnetic disturbances are closely related with the interplanetary magnetic field, particularly the southward component (negative Bz), since such condition can lead to the energy tranfer from the solar wind into the Earth’s magnetosphere. The energy transfer can cause disturbance in geomagnetic field, which is represented by disturbance index Dst. The good correlation between the minimum values of Bz and Dst means that the stronger the magnetic field can lead to the stronger disturbance. However, the minimum of both parameter do not occur simultaneously. From analysis of 41 geomagnetic storms with Dst ≤ -30 nT, in general, the time delay between Bz and Dst is two hours, which Bz reach minimum two hour before the Dst. It represent the time that required by the disturbance to travel from magnetopause to the Earth. Keywords: Geomagnetic disturbance, Interplanetary magnetic field"

"Dalam tulisan ini dianalisa keterkaitan antara aktivitas matahari dengan aktivitas geomagnet yang teramati dari Stasiun Pengamat Dirgantara Biak untuk rentang waktu tahun 1996 sampai dengan 2001. Tingkat aktivitas matahari dinyatakan oleh indeks flare dan bilangan sunspot. Pengamatan aktivitas geomagnet dilakukan di Biak (koordinat geografis -1.08° lintang selatan dan 136.5° bujur timur, koordinat geomagnet -12.8° selatan). Ditunjukkan bahwa tingkat gangguan geomagnet akan naik bila aktivitas matahari juga meningkat, dan keduanya mempunyai korelasi yang baik pada malam hari waktu setempat."

"Pelontaran massa korona (CME) adalah salah satu aktivitas matahari yangmenghasilkan pancaran partikel energi tinggi ke angkasa. Partikel-partikel ini kemudian menjadi angin surya yang selanjutnya bisa mencapai bumi. Telaah ini mencoba melakukan analisis pada beberapa peristiwa CME yang cukup besar untuk bisa mendapatkan informasi mengenai pengaruh yang mungkin bisa diberikannya pada daerah-daerah yang cukup jauh melalui pancaran angin surya yang dihasilkannya. Untuk itu diamati juga gejala-gejala angin surya yang kemungkinan diakibatkan oleh CME tersebut. Didapat bahwa beberapa peristiwa CME menghasilkan angin surya yang cukup deras, tetapi ada juga yang tidak menghasilkan angin surya yang cukup deras. Perbedaan ini masih perlu ditelaah lebih lanjut dalam rangka mendapatkan gambaran yang lengkap mengenai adanya perbedaan-perbedaan tersebut."

"Flare observations are numerous, and this approach should be supported by theoretical approach especially through modelling by numerical simulation. We make an analysis of reconnection process which precedes flare through numerical simulation. This method is the best method in flare modelling because processes in flare behave non lineraly so analytical method can't be used."

"Three Long Duration Event (LDE) flares erupted from solar surface in the period of 15-17 January 2005. They have similar characteristics, which are gradual flares and reach maximum intensity longer than their decay. These LDE flares were accompanied by CME and proton event which led to the increase of 10.7 cm flux and to the local geomagnetic storms at middle and high latitude."

"In this paper we present the relationship between long duration H-alpha flare events and suspot number during the period of 1980-2004. We counted as long duration events all those of one hour or more. It is shown that the long duration H-alpha flare events tend to trace the sunspot cycle with some anomalies"

"Interplanetary structures are important for the development of geomagnetic disturbance. The structures include intense north-southward Interplanetary Magnetic Field, the shock, solar wind density and velocity, and probably the magnetic cloud. We studied five events of magnetic clouds which occurred in the minimum phase of solar activity in order to understand solar wind-magnetosphere coupling. The correlations between storm intensity and the different solar wind parameters will also be presented as well. By analyzing five magnetic clouds occurred in 2006 and the associated geomagnetic enhancement, we found that not all magnetic clouds lead to geomagnetic disturbances. "

"Tulisan ini berupa analisis kondisi atmosfer pada skala global dan regional pada tahun 2008. Berdasarkan data suhu permukaan dari NCDC (National Climatic Data Center), suhu permukaan bumi, baik daratan maupun lautan, pada tahun 2008, mengalami kenaikan sebesar 0,49ºC lebih tinggi dibandingkan dengan rata-rata suhu abad 20. Tercatat suhu-suhu ekstrim di tahun 2008 termasuk suhu di bawah rata-rata di wilayah Timur Tengah, Asia Tengah, China tenggara pada bulan Januari 2008. Berdasarkan data MSU yang dianalisis untuk NOAA oleh Universitas Alabama di Huntsville (UAH), Remote Sensing Systems (RSS, Santa Rosa, California) dan Universitas Washington (UW), ada kenaikan suhu global di troposfer tengah, meskipun menggunakan teknik analisis yang berbeda, tetapi memberikan hasil yang sama kecuali trendnya. Presipitasi global di tahun 2008 lebih tinggi dibandingkan dengan presipitasi rata-rata selama tahun 1961-1990. Presipitasi selama setahun bervariasi terhadap wilayah. Dalam skala regional, kondisi kering terjadi di Hawai, Amerika Serikat bagian barat dan tengah selatan, Alaska bagian barat daya, Afrika tenggara, Eropa selatan, India utara dan beberapa wilayah di Argentina, Uruguay, Asia Timur, sepanjang pantai timur Brazil dan Australia bagian barat daya. "

"hanges in the daily variation of H component due to magnetic storms with a duration of hours to days is the space weather information is very important for further decision making for the user. Activity disturbance caused wave/influx of energetic particles that arise through the solar wind, can solve the earth's magnetic field is strong at very short intervals. Changes in the daily variation H component is generally an increase or decrease up to hundreds of nano tesla from a stable ondition. In the paper be discussion analysis of changes in the daily variation of H component magnet during magnetic storms using double Fourier series. In order to obtain information from changes daily variation of H component during magnetic storms through data from monitoring stations geomagnetic Biak and Tangerang. The results of analysis obtained 3 times a magnetic storm events occur fluctuation SSG to daily variations in H component in Tangerang April 2001, in order 171nT,-and-125nT 221nT. Magnetic storm SSC 28 April 2001 showed changes occur daily variation of H component in the station at Biak -467nT and 1124nT."

"Periodic magnetic storms are those related to reccurent coronal hole events within a period of one solar rotation. There are still few studies on successive periodic magnetic storm. In this paper, we discuss the nature of the amplitude of the periodic magnetic storms within the solar cycle 20,21,22, and 23. The periodic nature of solar wind ( 27 days) occured on descending phase of solar cycle 22 also caused a reccurent geomagnetic disturbance. The disturbance developed into a geomagnetic storm in the first (27 days) and the ninth rotation. The geomegnetic disturbances with period 27 and 13.5 days are both significant at the low latitude while the period of 30 days are more dominant at the high latitude. That mean, from two flows of high velicity plasmas, only one that higher contribution on the occurence of geomagnetic disturbance accompanied by high intensity southern Bz field."