Search Results - "Ramelli, Renzo"
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1
Reconstruction of the Sunspot Number Source Database and the 1947 Zurich Discontinuity
Published in Solar physics (01-09-2021)“…The recalibration of the sunspot number series, the primary long-term record of the solar cycle, requires the recovery of the entire collection of raw sunspot…”
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2
Robotic and Non-Robotic Control of Astrophysical Instruments
Published in Advances in astronomy (01-01-2010)“…We present a system of device control programs, developed for the solar observatory at Locarno/Switzerland (IRSOL). Because these programs are implemented as…”
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3
Sunspot Observations and Counting at Specola Solare Ticinese in Locarno Since 1957
Published in Solar physics (01-11-2016)“…Specola Solare Ticinese is an observatory dedicated to sunspot number counting. It was constructed in 1957 in Locarno, Southern Switzerland, as an external…”
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4
Reconstruction of the Sunspot Number Source Database and the 1947 Zurich Discontinuity
Published 06-01-2023“…Solar Physics, Volume 296, Issue 9, article id.137, 2021 The recalibration of the sunspot number series, the primary long-term record of the solar cycle,…”
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5
Hanle rotation signatures in Sr I 4607 {\AA}
Published 06-05-2022“…A&A 662, A46 (2022) Observations of scattering polarization and the Hanle effect in various spectral lines are increasingly used to complement traditional…”
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6
Robotic and Non-Robotic Control of Astrophysical Instruments
Published in Advances in astronomy (2010)“…We present a system of device control programs, developed for the solar observatory at Locarno/Switzerland (IRSOL). Because these programs are implemented as…”
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7
Characterization of a thinned back illuminated MIMOSA V sensor as a visible light camera
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (01-09-2006)“…This paper reports the measurements that have been performed both in the Silicon Detector Laboratory at the University of Insubria (Como, Italy) and at the…”
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8
Sunspot data collection of Specola Solare Ticinese in Locarno
Published 23-05-2018“…Sunspot observations and counting are carried out at the Specola Solare Ticinese in Locarno since 1957 when it was built as an external observing station of…”
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9
Measurement of the evolution of the magnetic field of the quiet photosphere during a solar cycle
Published 10-08-2017“…The solar photosphere is filled by a magnetic field which is tangled on scales much smaller than the resolution capability of solar telescopes. This hidden…”
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Observations on spatial variations of the Sr~{\sc i} 4607~\AA~scattering polarization signals at different limb distances with ZIMPOL
Published 09-08-2019“…The Sr~{\sc i} 4607~\AA\ spectral line shows one of the strongest scattering polarization signals in the visible solar spectrum. The amplitude of this…”
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11
Spatial variations of the SrI 4607\AA scattering polarization signals at subgranular scale observed with ZIMPOL at GREGOR telescope
Published 08-04-2019“…Sr I 4607\AA spectral line shows one of the strongest scattering polarization signals in the visible solar spectrum. The amplitudes of these signals are…”
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12
Sunspot Observations and Counting at Specola Solare Ticinese in Locarno since 1957
Published 25-02-2016“…Specola Solare Ticinese is an observatory dedicated to Sunspot Number counting, which was constructed in 1957 in Locarno, Southern Switzerland, as an external…”
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13
Helium Emissions Observed in Ground-Based Spectra of Solar Prominences
Published 02-10-2012“…2012SoPh..281..697W The only prominent line of singly ionized helium in the visible spectral range, helium-II 4686 A, is observed together with the helium-I…”
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14
He-D3 Polarization observed in Prominences
Published 23-01-2004“…Spectro-polarimetric measurements of the D3-HeI 5876 A line profile in 35 prominences have been performed in 2003 with the Gregory-Coud\'e Telescope in…”
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15
Scattering polarization and the Hanle effect in H-alpha as a probe of chromospheric magnetism: Modeling vs. Observations
Published 24-02-2011“…The Hanle effect in strong spectral lines is the physical mechanism that should be increasingly exploited for quantitative explorations of the magnetism of the…”
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16
The power spectrum of the seeing during solar observations
Published 02-12-2011“…Measurements of the power spectrum of the atmospheric seeing in the line of sight of the Sun, in the range 0.001-1 Hz, have been performed in Santa Maria degli…”
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17
Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements
Published 28-12-2011“…Measurements of the power spectrum of the seeing in the range 0.001-1 Hz have been performed in order to understand the criticity of the transits' method for…”
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