امان از این همه جوونه که گل کرد تو خلا و ما که خوابمون سبک بود افتادیم از گهواره های تاریخ اما روی صورت و صورتک ساختیم از زمین کدورت...

A near-infrared image of the Cosmic Cliffs in the Carina Nebula, captured by NASA’s Webb Telescope, has been mapped to a symphony of sounds. This track includes sounds from just the top half of the image, which resembles a dark blue night sky. The gas and dust that are represented in blue hues have been translated to windy, drone-like sounds. The sonification scans the image from left to right.
 
This sonification does not represent sounds recorded in space. Two musicians mapped the telescope’s data to sound, carefully composing music to accurately represent details the team would like listeners to focus on. In a way, this sonification is like modern dance or an impressionist painting – it converts Webb’s image to a new medium to engage and inspire listeners.

Brighter light in the image is louder. The vertical position of light also dictates the frequency of sound. For example, bright light near the top of the image sounds loud and high, but bright light near the bottom is loud and lower pitched.

Learn more: https://www.nasa.gov/feature/goddard/2022/nasa-webb-s-first-full-color-images-data-are-set-to-sound

Credits: Image: NASA, ESA, CSA, and STScI; Accessibility Production: NASA, ESA, CSA, STScI, and Kimberly Arcand (CXC/SAO), Matt Russo and Andrew Santaguida (SYSTEM Sounds), Quyen Hart (STScI), Claire Blome (STScI), and Christine Malec (consultant).

Webb’s Cosmic Cliffs Sonification: Sky

NASA’s Webb Telescope observed the atmospheric characteristics of the hot gas giant exoplanet WASP-96 b – which contains clear signatures of water – and the resulting transmission spectrum’s individual data points were translated into sound.
 
The sonification scans the spectrum from left to right. From bottom to top, the y-axis ranges from less to more light blocked. The x-axis ranges from 0.6 microns on the left to 2.8 microns on the right. The pitches of each data point correspond to the frequencies of light each point represents. Longer wavelengths of light have lower frequencies and are heard as lower pitches. The volume indicates the amount of light detected in each data point. 
 
The four water signatures are represented by the sound of water droplets falling. These sounds simplify the data – water is detected as a signature that has multiple data points. The sounds align only to the highest points in the data.
 
Learn more: https://www.nasa.gov/feature/goddard/2022/nasa-webb-s-first-full-color-images-data-are-set-to-sound

Credits: Image: Image: NASA, ESA, CSA, and STScI; Accessibility Production: NASA, ESA, CSA, STScI, and Kimberly Arcand (CXC/SAO), Matt Russo and Andrew Santaguida (SYSTEM Sounds), Quyen Hart (STScI), Claire Blome (STScI), and Christine Malec (consultant).

Webb’s Exoplanet WASP-96 b Sonification

NASA’s InSight lander brought a seismometer to the Red Planet to study “marsquakes.” On Sept, 5, 2021, the seismometer detected a meteoroid impacting the planet’s surface, creating several craters in the process.
It was the first time the sound of a meteoroid impact was captured occurring on another planet, and it might not be what you expect. In the audio, you hear three “bloops” representing distinct moments of the impact: the meteoroid entering Mars’ atmosphere, exploding into pieces, and striking the ground. The peculiar sound is caused by an atmospheric effect that’s also been observed in deserts on Earth, where lower-pitched sounds arrive before high-pitched sounds.
Credit: CNES/IPGP

InSight Captures Sound of a Meteoroid Striking Mars

This sonification is of the signals recorded by NASA’s InSight Mars lander, which detected a giant meteoroid strike on Dec. 24, 2021, the 1,094th Martian day, or sol, of the mission. InSight’s seismometer records seismic signals that are not in the range of human hearing. In order to make the signals audible, the data was sped up 100 times.
Credit: NASA/JPL-Caltech/CNES/Imperial College London

NASA’s InSight Records the Sound of a Martian Impact

This audio shows the results of NASA’s Perseverance Mars rover using its SuperCam microphone to record the sounds of a Martian dust devil – the first time any such recording has been made. The dust devil passed directly over Perseverance on Sept. 27, 2021, the 215th Martian day, or sol, of the mission.
Credit: NASA/JPL-Caltech/LANL/CNES/CNRS/INTA-CSIC/Space Science Institute/ISAE-Supaero

NASA's Perseverance Records a Martian Dust Devil

One year ago, the Hunga Tonga-Hunga Ha’apai volcano erupted, causing widespread destruction to the Pacific Island Nation of Tonga. It spewed volcanic material up to 58 km into the atmosphere, brought a nearly 15 m tsunami that crashed ashore, destroying villages, and created a sonic boom that rippled around the world – twice. 

Even one year on, interest in the extraordinary explosive eruption remains. A sound artist has recently recreated the sonification of the underwater volcanic eruption using rayleigh signal intensity data provided by the Aeolus Virtual Research Environment platform.

Using wind data obtained on one of its overpasses over the ash cloud of the Hunga Tonga explosion, Jamie Perera used an audio sample of one of the shock waves, time-stretched it into a ghostly tone, and assigned it to harmonic values transcribed from 90 Aeolus readings taken over a duration of approximately 15 minutes. 
The listener hears one reading every two seconds, in a harmonic range that spans six piano octaves, the highest of which can be heard at around 01:18 minutes when the readings show the eruption’s dust plume at its highest peak (over 20.5 km). The artistic intention behind the sonification was to evoke the otherworldly landscape of Hunga Tonga and other volcanoes. 

Sonification credit/copyright: @jamieperera (2023). Used by permission. Data and guidance provided by Daniel Santillan. Thanks to Peter Bickerton and Jemma Foster. Originally created as part of Wild Alchemy Journal - Air Edition - Aeolus

Sound of the Hunga Tonga Volcanic Eruption

Between Earth and the Sun, space is not truly empty but is filled with a soup of charged particles called plasma. This plasma comes from the Sun, pumped out in a steady stream called the solar wind and sporadically blasted away in explosive solar eruptions. When this solar plasma strikes Earth, it causes the magnetic field lines and plasma around Earth to vibrate like the plucked strings of a harp, producing ultralow-frequency waves.

In 2007, NASA launched five satellites to fly through Earth’s magnetic “harp” – its magnetosphere – as part of the THEMIS mission (Time History of Events and Macroscale Interactions during Substorms). Since then, THEMIS has been gathering a bounty of information about plasma waves across Earth’s magnetosphere. 

The frequencies of the waves THEMIS measures are too low for our ears to hear, however. So a NASA citizen science project called HARP – or Heliophysics Audified: Resonances in Plasmas – has sped up the waves recorded by THEMIS to convert them to sound waves.

In this clip from March 2-5, 2012, whistle sounds are repeatedly heard over ambient background whooshes and crunches. The whistles change in pitch as a THEMIS spacecraft moves toward and away from Earth on three orbits, with a maximum altitude of about 50,000 miles. These sounds are related to Earth’s magnetic harp, which has longer magnetic strings and lower pitches farther away from Earth. These three orbits happened when the solar wind was relatively quiet, but it’s still able to pluck the strings of Earth’s magnetic harp while also causing many other types of magnetic vibrations, most of which sound like background whooshes and crunches.

Multiple Passes through the Magnetospheric Harp on March 2-5, 2012

Courtesty of Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS)aboard NASA’s Van Allen Probes team at the University of Iowa

Chorus Radio Waves within Earth's Atmosphere

Sputnik: Beep

Another gem from the ESA archives: 

Tracks left behind by the November 2000 Leonids shower, as detected by ESA scientists.

Each time a meteor crosses the atmosphere, it leaves behind a short trail of ionised particles. This trail reflects high-frequency radio signals from stations around the world for just a few seconds. The motion of the meteor trail due to the upper atmosphere winds changes the frequency of the reflected signal (Doppler effect). You 'hear' the trail as it is blown around by the winds before it is eventually dispersed.

You are invited to use, re-use or remix this sonification. When doing so, please credit 'ESA - European Space Agency, CC BY-SA 3.0 IGO' and stick to the licence:

This work is licenced under the Creative Commons Attribution-ShareAlike 3.0 IGO (CC BY-SA 3.0 IGO) licence. The user is allowed to reproduce, distribute, adapt, translate and publicly perform this publication, without explicit permission, provided that the content is accompanied by an acknowledgement that the source is credited as 'ESA - European Space Agency’, a direct link to the licence text is provided and that it is clearly indicated if changes were made to the original content. Adaptation/translation/derivatives must be distributed under the same licence terms as this publication. The user must not give any suggestion that ESA necessarily endorses the modifications that you have made.

No warranties are given. The license may not give you all of the permissions necessary for your intended use. For example, other rights such as publicity, privacy, or moral rights may limit how you use the material.

Any of the above conditions can be waived if you get permission from ESA. To view a copy of this license, please visit http://creativecommons.org/licenses/by-sa/3.0/igo/

Source: http://www.esa.int/Our_Activities/Space_Science/Sounds_from_space 

Wailing Leonids

A subwoofer or earphones are needed to hear this clip. Listen to raw, unprocessed data from the seismometer on NASA's InSight spacecraft of vibrations caused by wind moving over the solar panels on Mars. The sounds were recorded by two of the three short-period sensors on the seismometer (SEIS). 
 
JPL manages InSight for NASA's Science Mission Directorate. InSight is part of NASA's Discovery Program, managed by the agency's Marshall Space Flight Center in Huntsville, Alabama.
 
France’s national space agency, Centre National d’Études Spatiales (CNES), Paris, leads the consortium that provided SEIS. The principal investigator for SEIS is Philippe Lognonné of the Institute of Earth Physics of Paris (Institut de Physique du Globe de Paris, or IPGP). Imperial College, London, and Oxford University made the short-period sensors.
 
For more information on the InSight mission, visit https://mars.nasa.gov/insight
 
Credit: NASA/JPL-Caltech/CNES/UKSA/Imperial College London/Oxford/ETH

Raw Sounds from InSight's Seismometer on Mars (full length)

Hello, we’re NASA. You may have seen our astronauts, rocket launches, or Mars rovers — but have you heard our sounds? From interviews with astronauts and engineers to stories that take you on a tour of the galaxy, NASA’s audio offerings let you experience the thrill of space exploration without ever leaving Earth.

NASA’s InSight Records the Sound of a Martian Impact

NASA

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