Search results for "Sunrise"

showing 10 items of 25 documents

Analytic continuation and numerical evaluation of the kite integral and the equal mass sunrise integral

2017

We study the analytic continuation of Feynman integrals from the kite family, expressed in terms of elliptic generalisations of (multiple) polylogarithms. Expressed in this way, the Feynman integrals are functions of two periods of an elliptic curve. We show that all what is required is just the analytic continuation of these two periods. We present an explicit formula for the two periods for all values of $t \in {\mathbb R}$. Furthermore, the nome $q$ of the elliptic curve satisfies over the complete range in $t$ the inequality $|q|\le 1$, where $|q|=1$ is attained only at the singular points $t\in\{m^2,9m^2,\infty\}$. This ensures the convergence of the $q$-series expansion of the $\mathr…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsPure mathematics010308 nuclear & particles physicsFeynman integralAnalytic continuationFOS: Physical sciencesMathematical Physics (math-ph)01 natural sciencesElliptic curveRange (mathematics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)NomeKite0103 physical sciencesConvergence (routing)Sunriselcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsMathematical PhysicsNuclear Physics B
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COMPARISON BETWEEN Mg IIkAND Ca II H IMAGES RECORDED BY SUNRISE/SuFI

2014

We present a comparison of high-resolution images of the solar surface taken in the Mg II k and Ca II H channels of the Filter Imager on the balloon-borne solar observatory SUNRISE. The Mg and Ca lines are sampled with 0.48 nm and 0.11 nm wide filters, respectively. The two channels show remarkable qualitative and quantitative similarities in the quiet Sun, in an active region plage and during a small flare. However, the Mg filtergrams display 1.4-1.7 times higher intensity contrast and appear more smeared and smoothed in the quiet Sun. In addition, the fibrils in a plage are wider. Although the exposure time is 100 times longer for Mg images, the evidence suggests that these differences ca…

PhysicsPlageSolar observatorySpace and Planetary SciencelawSunriseAstronomy and AstrophysicsSolar surfaceAstrophysicsChromosphereFlarelaw.inventionThe Astrophysical Journal
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FULLY RESOLVED QUIET-SUN MAGNETIC FLUX TUBE OBSERVED WITH THE SUNRISE/IMAX INSTRUMENT

2010

Until today, the small size of magnetic elements in quiet Sun areas has required the application of indirect methods, such as the line-ratio technique or multi-component inversions, to infer their physical properties. A consistent match to the observed Stokes profiles could only be obtained by introducing a magnetic filling factor that specifies the fraction of the observed pixel filled with magnetic field. Here, we investigate the properties of a small magnetic patch in the quiet Sun observed with the IMaX magnetograph on board the balloon-borne telescope Sunrise with unprecedented spatial resolution and low instrumental stray light. We apply an inversion technique based on the numerical s…

PhysicsPhotosphereFlux tubeStray lightFOS: Physical sciencesAstronomy and AstrophysicsField strengthAstrophysicsMagnetic fluxMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceRadiative transferAstrophysics::Solar and Stellar AstrophysicsSunriseSolar and Stellar Astrophysics (astro-ph.SR)The Astrophysical Journal
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Photospheric response to an ellerman bomb-like event—an analogy of Sunrise/IMaX observations and MHD simulations

2017

S. Danilovic et. al.

PhysicsPhotosphere010504 meteorology & atmospheric sciencesphotosphere [Sun]Event (relativity)photometric [Techniques]Sun: photosphereAnalogyAstronomyAstronomy and AstrophysicsAstrophysics7. Clean energy01 natural sciencesmagnetic fields [Sun]Sun: activitySpace and Planetary Science0103 physical sciencesSunriseactivity [Sun]MagnetohydrodynamicsSun: magnetic fields010303 astronomy & astrophysicsChromosphereTechniques: photometric0105 earth and related environmental sciences
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Diurnal timing of nonmigratory movement by birds: the importance of foraging spatial scales

2020

Timing of activity can reveal an organism's efforts to optimize foraging either by minimizing energy loss through passive movement or by maximizing energetic gain through foraging. Here, we assess whether signals of either of these strategies are detectable in the timing of activity of daily, local movements by birds. We compare the similarities of timing of movement activity among species using six temporal variables: start of activity relative to sunrise, end of activity relative to sunset, relative speed at midday, number of movement bouts, bout duration and proportion of active daytime hours. We test for the influence of flight mode and foraging habitat on the timing of movement activit…

0106 biological sciencesDaytimeflight modetemporalForagingZoologyBiologySunsetTemporalnonmigratory01 natural sciences010605 ornithologyforagingMovement ecologyflight mode foraging movement ecology multispecies nonmigratory temporalddc:570SunriseNonmigratoryZoologíaDaylightForagingEcology Evolution Behavior and SystematicsFlight modeMovement (music)MultispeciesPelagic zoneDidáctica de las Ciencias ExperimentalesmultispeciesHabitatmovement ecologyAnimal Science and ZoologyEnvironmental Sciences
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Surface waves in solar granulation observed with {\sc Sunrise}

2010

Solar oscillations are expected to be excited by turbulent flows in the intergranular lanes near the solar surface. Time series recorded by the IMaX instrument aboard the {\sc Sunrise} observatory reveal solar oscillations at high resolution, which allow studying the properties of oscillations with short wavelengths. We analyze two times series with synchronous recordings of Doppler velocity and continuum intensity images with durations of 32\thinspace min and 23\thinspace min, resp., recorded close to the disk center of the Sun to study the propagation and excitation of solar acoustic oscillations. In the Doppler velocity data, both the standing acoustic waves and the short-lived, high-deg…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAcoustic waveComputational physicsStanding waveSuperposition principleWavelengthAmplitudeAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSurface waveSunriseWavenumberAstrophysics::Solar and Stellar AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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A tale of two emergences: Sunrise II observations of emergence sites in a solar active region

2017

R. Centeno et. al.

010504 meteorology & atmospheric sciencesField (physics)photosphere [Sun]Field lineFOS: Physical sciencesFluxchromosphere [Sun]Astrophysicspolarimetric [Techniques]01 natural sciences0103 physical sciencesSunrise010303 astronomy & astrophysicsChromosphereSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSunspotsSun: chromosphereTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsMagnetic reconnectionMagnetic fluxMagnetic fieldmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science
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The sunrise integral and elliptic polylogarithms

2016

We summarize recent computations with a class of elliptic generalizations of polylogarithms, arising from the massive sunrise integral. For the case of arbitrary masses we obtain results in two and four space-time dimensions. The iterated integral structure of our functions allows us to furthermore compute the equal mass case to arbitrary order.

High Energy Physics - TheoryClass (set theory)Pure mathematicsDifferential formDifferential equationComputationFOS: Physical sciencesOrder (ring theory)Feynman graphHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Iterated integralsSunriseMathematicsProceedings of Loops and Legs in Quantum Field Theory — PoS(LL2016)
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Oscillations on Width and Intensity of Slender Ca ii H Fibrils from Sunrise/SuFI

2017

R. Gafeira et. al.

010504 meteorology & atmospheric sciencesPhase (waves)FOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencesMolecular physics0103 physical sciencesWave modeSunriseSun: oscillationsTechniques: imaging spectroscopySun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSolar observatoryoscillations [Sun]imaging spectroscopy [Techniques]Sun: chromosphereAstronomy and AstrophysicsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]Space and Planetary ScienceIntensity (heat transfer)The Astrophysical Journal Supplement Series
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Supersonic Magnetic Upflows in Granular Cells Observed with Sunrise/IMaX

2010

Using the IMaX instrument on-board the Sunrise stratospheric balloon-telescope we have detected extremely shifted polarization signals around the Fe I 5250.217 {\AA} spectral line within granules in the solar photosphere. We interpret the velocities associated with these events as corresponding to supersonic and magnetic upflows. In addition, they are also related to the appearance of opposite polarities and highly inclined magnetic fields. This suggests that they are produced by the reconnection of emerging magnetic loops through granular upflows. The events occupy an average area of 0.046 arcsec$^2$ and last for about 80 seconds, with larger events having longer lifetimes. These supersoni…

PhysicsPhotosphereMagnetismStellar atmosphereFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSpectral lineMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSunriseSupersonic speedSolar and Stellar Astrophysics (astro-ph.SR)Main sequence
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