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    <title>NISCAIR Online Periodicals Repository Collection: IJRSP Vol.39(5) [October 2010]</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10599</link>
    <description>&lt;b&gt;Includes papers from IHY workshop Nainital&lt;/b&gt;</description>
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  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10618">
    <title>Study of upper atmospheric emissions using Mesosphere Lower Thermosphere Photometer (MLTP) designed at ARIES</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10618</link>
    <description>Title: Study of upper atmospheric emissions using Mesosphere Lower Thermosphere Photometer (MLTP) designed at ARIES
&lt;br/&gt;
&lt;br/&gt;Authors: Bangia, T; Bhattacharjee, S; Guharay, A; Taori, A; Uddin, Wahab
&lt;br/&gt;
&lt;br/&gt;Abstract: Mesosphere&#xD;
Lower Thermosphere Photometer (MLTP) has been designed at ARIES for studying&#xD;
mesosphere lower thermosphere coupling processes. MLTP utilizes f/2 optics with&#xD;
4&lt;sup&gt;o&lt;/sup&gt; circular field of view. It has seven narrow bandwidth (FWHM ~ 4&#xD;
Å) interference filters mounted on a geared filter plate housed in filter&#xD;
chamber under precise temperature controlled conditions. Out of these seven&#xD;
filters, filter at 630 nm is meant to monitor ionospheric F- region airglow&#xD;
emission due to atomic oxygen. MLTP has been successfully installed and made&#xD;
operational at Space Weather Laboratory of ARIES.
&lt;br/&gt;
&lt;br/&gt;Page(s): 325-329</description>
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  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10617">
    <title>Solar Vector Magnetograph: Instrument status and vector field measurements of non-flaring solar active regions</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10617</link>
    <description>Title: Solar Vector Magnetograph: Instrument status and vector field measurements of non-flaring solar active regions
&lt;br/&gt;
&lt;br/&gt;Authors: Gosain, Sanjay; Venkatakrishnan, P
&lt;br/&gt;
&lt;br/&gt;Abstract: The&#xD;
Solar Vector Magnetograph (SVM) of Udaipur Solar Observatory (USO) is an&#xD;
imaging polarimeter based on a tunable Fabry-Perot filter. In the present&#xD;
paper, the development efforts during phase-II of this instrument have been&#xD;
presented. These include: (i) installation of the instrument on a new robotic&#xD;
mount at the island site of USO; (ii) polarimetric calibrations of the&#xD;
instrument; and (iii) development of tools for performing data reduction and Stokes&#xD;
inversion. In particular, the Milne-Eddington inversion of polarized line&#xD;
profiles of the entire active region using parallel computing concept is&#xD;
described. Finally, few preliminary results regarding the vector magnetic field&#xD;
and other activity parameters of sunspots in non-flaring solar active regions&#xD;
are discussed. Such observations serve as a reference for comparison with&#xD;
flaring active regions.
&lt;br/&gt;
&lt;br/&gt;Page(s): 319-324</description>
  </item>
  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10616">
    <title>A Dual beam H&lt;img src='/image/spc_char/alpha.gif' border=0&gt; Doppler system to acquire, analyse and anticipate solar eruptive events directed towards Earth</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10616</link>
    <description>Title: A Dual beam H&lt;img src='/image/spc_char/alpha.gif' border=0&gt; Doppler system to acquire, analyse and anticipate solar eruptive events directed towards Earth
&lt;br/&gt;
&lt;br/&gt;Authors: Joshi, Anand D; Mathew, Shibu K; Srivastava, Nandita; Martin, Sara F; Gupta, Sudhir Kumar
&lt;br/&gt;
&lt;br/&gt;Abstract: A new&#xD;
instrument with a dual-beam Hα Doppler system is being developed at the Udaipur&#xD;
Solar Observatory (USO) &#xD;
in order to improve the quality and quantity of data on quiet, activated and&#xD;
erupting filaments and prominences on the &#xD;
Sun, especially those associated with geo-effective coronal mass ejections.&#xD;
These data can be potentially used to construct three-dimensional topology of&#xD;
erupting filaments as they leave the surface of the Sun and can be compared&#xD;
with &#xD;
multi-wavelength data obtained from space missions such as STEREO, SOHO and Hinode. The characterization of various optical&#xD;
components for the instrument is being carried out, and some preliminary&#xD;
results are presented in the paper.
&lt;br/&gt;
&lt;br/&gt;Page(s): 315-318</description>
  </item>
  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10615">
    <title>Influence of solar variability on rainwater</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10615</link>
    <description>Title: Influence of solar variability on rainwater
&lt;br/&gt;
&lt;br/&gt;Authors: Joshi, Indira Sudhir
&lt;br/&gt;
&lt;br/&gt;Abstract: The&#xD;
significant effect of the high-energy charged particles, entering the earth’s&#xD;
environment from interplanetary space, on the space and terrestrial weather is&#xD;
well known. Solar flares emit electron particles. These electrons interact with&#xD;
Earth’s magnetic field and atmosphere causing weather, geophysical and&#xD;
behavioural changes. These charged particles from the sun affect Earth’s&#xD;
magnetic field and increase atmospheric nucleation which then affects cloud&#xD;
formation and thus the weather. Keeping this in view, a study has been undertaken&#xD;
to examine the changes in rainwater associated with the high energy charged&#xD;
particles entering the earth’s environment from interplanetary space. It is&#xD;
observed from the analysis that an increase in proton and electron fluences is&#xD;
followed by an increase in electrical conductivity and decrease in pH of&#xD;
rainwater over Pune.
&lt;br/&gt;
&lt;br/&gt;Page(s): 312-314</description>
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