Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

Flame Photometry: Overview01:02

Flame Photometry: Overview

Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
Light Acquisition02:16

Light Acquisition

In order to produce glucose, plants need to capture sufficient light energy. Many modern plants have evolved leaves specialized for light acquisition. Leaves can be only millimeters in width or tens of meters wide, depending on the environment. Due to competition for sunlight, evolution has driven the evolution of increasingly larger leaves and taller plants, to avoid shading by their neighbors with contaminant elaboration of root architecture and mechanisms to transport water and nutrients.
Focusing of Light in the Eye01:16

Focusing of Light in the Eye

Light rays enter the eye through the cornea, a transparent dome-shaped tissue that is the eye's outermost layer. The cornea bends or refracts, light rays traveling to the pupil. The shape of the cornea determines how much of the light is bent and whether the image will be focused correctly on the retina at the back of the eye. Once the light has passed through both refraction layers, it converges into a single focal point onto a small area. This is where photoreceptors start transforming...
Flame Photometry: Lab01:16

Flame Photometry: Lab

In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

DNA-based vaccination against hepatitis B virus using dissolving microneedle arrays adjuvanted by cationic liposomes and CpG ODN.

Drug delivery·2015
Same author

[Correlations between DNA mismatch repair (MMR) and prognosis and prediction of treatment efficacy in stage II/II colon cancer].

Zhonghua zhong liu za zhi [Chinese journal of oncology]·2015
Same author

[Clinical effect of hemoperfusion combined with hemodialysis in treatment of severe organophosphate pesticide poisoning].

Zhonghua lao dong wei sheng zhi ye bing za zhi = Zhonghua laodong weisheng zhiyebing zazhi = Chinese journal of industrial hygiene and occupational diseases·2015
Same author

Effect of orexin A on apoptosis in BGC-823 gastric cancer cells via OX1R through the AKT signaling pathway.

Molecular medicine reports·2015
Same author

Time-resolved dynamic dilution introduction for ion mobility spectrometry and its application in end-tidal propofol monitoring.

Journal of breath research·2015
Same author

Curative effect assessment of bandage contact lens in neurogenic keratitis.

International journal of ophthalmology·2014

Related Experiment Video

Updated: May 20, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Blurred star image processing for star sensors under dynamic conditions.

Weina Zhang1, Wei Quan, Lei Guo

  • 1Science and Technology on Inertial Laboratory, Key Laboratory of Fundamental Science for National Defense-Novel Inertial Instrument & Navigation System Technology, Beijing 100191, China. yuzhanglina@yahoo.com.cn

Sensors (Basel, Switzerland)
|July 11, 2012
PubMed
Summary
This summary is machine-generated.

This study introduces a new method to improve star sensor accuracy under dynamic conditions. It effectively denoises and restores blurred star images, crucial for satellite attitude determination.

Keywords:
dynamic conditionsimage denoisingimage restorationstar sensor

More Related Videos

Test Samples for Optimizing STORM Super-Resolution Microscopy
16:52

Test Samples for Optimizing STORM Super-Resolution Microscopy

Published on: September 6, 2013

Related Experiment Videos

Last Updated: May 20, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Test Samples for Optimizing STORM Super-Resolution Microscopy
16:52

Test Samples for Optimizing STORM Super-Resolution Microscopy

Published on: September 6, 2013

Area of Science:

  • Aerospace Engineering
  • Image Processing
  • Astrodynamics

Background:

  • Precise star point location is critical for star sensors in identifying star maps and determining aircraft attitude.
  • Dynamic conditions, such as high angular rates, introduce noise and motion blur to star images, degrading sensor performance.
  • Existing methods struggle to effectively process blurred star images acquired under dynamic conditions.

Purpose of the Study:

  • To propose a novel method for processing blurred star images acquired by star sensors under dynamic conditions.
  • To enhance the precision of star point location for improved attitude determination.
  • To address the challenges posed by noise and motion blur in star images.

Main Methods:

  • A denoising method utilizing an adaptive wavelet threshold is employed for noisy star images.
  • A restoration method based on a deduced mathematical model of motion blur is applied for large angular rates.
  • The proposed method integrates denoising and restoration tailored to different angular rate conditions.

Main Results:

  • Simulation results demonstrate the effectiveness of the proposed adaptive denoising and motion blur restoration technique.
  • The method successfully processes blurred star images corrupted by noise and motion under dynamic conditions.
  • Validated improvements in star point location accuracy and overall star sensor performance.

Conclusions:

  • The developed method is effective for processing blurred star images under dynamic conditions.
  • It offers a practical solution for enhancing the attitude determination accuracy of satellites.
  • The approach provides a significant advancement in star sensor technology for dynamic environments.