Tidal synchronous orbit: A novel approach to remote sensing of oceanic regions

Research output: Contribution to conferencePoster

Abstract

To-date space-based remote sensing of oceans and coastal regions has principally been conducted from platforms in Sun-Synchronous Low Earth Orbit (LEO). Such a trajectory, while beneficial in terms of solar illumination angle, has limitations in that geometric patterns driven primarily by tidal variation (such as coastal bathymetry and suspended sediment reflectance) may not be captured effectively. As such, tidal-synchronous observations can be expected to provide enhanced remote sensing of oceanic regions where tidal variation plays a key role. This paper introduces the concept of Tidal synchronism, defining it as when the orbit period of a platform is synchronised with the rotation period of the Earth such that a repeat ground-track is achieved after an integer number of ‘tidal periods’ (twice the ‘principal lunar semi-diurnal’ constituent). Such a Tidal-Synchronous platform would facilitate analysis of specific locations, at specific times in the regular tidal sequence, resulting in improved monitoring of evolving patterns as a function of tidal variation. Whilst a Sun-Synchronous orbit has been necessary for the majority of large, multi-functional Earth Observation platforms (e.g. ENVISAT), specific mission applications realised through smaller, specialised technologies are becoming increasingly common, for which a tidal synchronous orbit is found to be beneficial.

For the first time, this paper introduces the concept of a Tidal-Synchronous orbit and describes the astrodynamic properties of such a trajectory under the influence of natural perturbations (J2) via a set of Modified Equinoctial Elements. Analytical solutions for low thrust propulsive station-keeping are presented, for the general case of orbit and repeat parameter combinations, indicating the applicability of such a mission to small, resource limited spacecraft. It is shown that a repeat ground-track can be achieved every 28 tidal periods with a single platform, through exploitation of natural perturbations alone (imager field of view would govern temporal resolution over any given region). A constellation of satellites could be deployed to achieve greater temporal resolution (additional satellites in an orbit plane) and greater number of ground-track repeats at specific tidal times (additional orbit planes). It is also shown that orbit parameters attributed to a repeat ground-track after exactly 57 tidal periods are almost identical to those required for a Sun-Synchronous orbit (approximately 5deg drift in relative solar angle per year). In this case, benefits from each class of synchronism could be exploited in order to achieve high quality, reliable visible imaging data at regular times in the tidal sequence.
LanguageEnglish
PagesIAC-12-B1.2.17 p13924
Publication statusPublished - 1 Oct 2012
Event63rd International Astronautical Congress - Naples, Italy
Duration: 1 Oct 20125 Oct 2012

Conference

Conference63rd International Astronautical Congress
CountryItaly
CityNaples
Period1/10/125/10/12

Fingerprint

Remote sensing
Orbits
Sun
Earth (planet)
Synchronization
Trajectories
Satellites
Bathymetry
Suspended sediments
Space flight
Image sensors
Spacecraft
Lighting
Imaging techniques
Monitoring

Keywords

  • orbit determination
  • remote sensing applications
  • oceanic data

Cite this

Lowe, C., Macdonald, M., Greenland, S. C., & McKee, D. (2012). Tidal synchronous orbit: A novel approach to remote sensing of oceanic regions. IAC-12-B1.2.17 p13924. Poster session presented at 63rd International Astronautical Congress, Naples, Italy.
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Lowe, C, Macdonald, M, Greenland, SC & McKee, D 2012, 'Tidal synchronous orbit: A novel approach to remote sensing of oceanic regions' 63rd International Astronautical Congress, Naples, Italy, 1/10/12 - 5/10/12, pp. IAC-12-B1.2.17 p13924.

Tidal synchronous orbit : A novel approach to remote sensing of oceanic regions. / Lowe, Christopher; Macdonald, Malcolm; Greenland, Stephen Charles; McKee, David.

2012. IAC-12-B1.2.17 p13924 Poster session presented at 63rd International Astronautical Congress, Naples, Italy.

Research output: Contribution to conferencePoster

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T1 - Tidal synchronous orbit

T2 - A novel approach to remote sensing of oceanic regions

AU - Lowe, Christopher

AU - Macdonald, Malcolm

AU - Greenland, Stephen Charles

AU - McKee, David

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Y1 - 2012/10/1

N2 - To-date space-based remote sensing of oceans and coastal regions has principally been conducted from platforms in Sun-Synchronous Low Earth Orbit (LEO). Such a trajectory, while beneficial in terms of solar illumination angle, has limitations in that geometric patterns driven primarily by tidal variation (such as coastal bathymetry and suspended sediment reflectance) may not be captured effectively. As such, tidal-synchronous observations can be expected to provide enhanced remote sensing of oceanic regions where tidal variation plays a key role. This paper introduces the concept of Tidal synchronism, defining it as when the orbit period of a platform is synchronised with the rotation period of the Earth such that a repeat ground-track is achieved after an integer number of ‘tidal periods’ (twice the ‘principal lunar semi-diurnal’ constituent). Such a Tidal-Synchronous platform would facilitate analysis of specific locations, at specific times in the regular tidal sequence, resulting in improved monitoring of evolving patterns as a function of tidal variation. Whilst a Sun-Synchronous orbit has been necessary for the majority of large, multi-functional Earth Observation platforms (e.g. ENVISAT), specific mission applications realised through smaller, specialised technologies are becoming increasingly common, for which a tidal synchronous orbit is found to be beneficial.For the first time, this paper introduces the concept of a Tidal-Synchronous orbit and describes the astrodynamic properties of such a trajectory under the influence of natural perturbations (J2) via a set of Modified Equinoctial Elements. Analytical solutions for low thrust propulsive station-keeping are presented, for the general case of orbit and repeat parameter combinations, indicating the applicability of such a mission to small, resource limited spacecraft. It is shown that a repeat ground-track can be achieved every 28 tidal periods with a single platform, through exploitation of natural perturbations alone (imager field of view would govern temporal resolution over any given region). A constellation of satellites could be deployed to achieve greater temporal resolution (additional satellites in an orbit plane) and greater number of ground-track repeats at specific tidal times (additional orbit planes). It is also shown that orbit parameters attributed to a repeat ground-track after exactly 57 tidal periods are almost identical to those required for a Sun-Synchronous orbit (approximately 5deg drift in relative solar angle per year). In this case, benefits from each class of synchronism could be exploited in order to achieve high quality, reliable visible imaging data at regular times in the tidal sequence.

AB - To-date space-based remote sensing of oceans and coastal regions has principally been conducted from platforms in Sun-Synchronous Low Earth Orbit (LEO). Such a trajectory, while beneficial in terms of solar illumination angle, has limitations in that geometric patterns driven primarily by tidal variation (such as coastal bathymetry and suspended sediment reflectance) may not be captured effectively. As such, tidal-synchronous observations can be expected to provide enhanced remote sensing of oceanic regions where tidal variation plays a key role. This paper introduces the concept of Tidal synchronism, defining it as when the orbit period of a platform is synchronised with the rotation period of the Earth such that a repeat ground-track is achieved after an integer number of ‘tidal periods’ (twice the ‘principal lunar semi-diurnal’ constituent). Such a Tidal-Synchronous platform would facilitate analysis of specific locations, at specific times in the regular tidal sequence, resulting in improved monitoring of evolving patterns as a function of tidal variation. Whilst a Sun-Synchronous orbit has been necessary for the majority of large, multi-functional Earth Observation platforms (e.g. ENVISAT), specific mission applications realised through smaller, specialised technologies are becoming increasingly common, for which a tidal synchronous orbit is found to be beneficial.For the first time, this paper introduces the concept of a Tidal-Synchronous orbit and describes the astrodynamic properties of such a trajectory under the influence of natural perturbations (J2) via a set of Modified Equinoctial Elements. Analytical solutions for low thrust propulsive station-keeping are presented, for the general case of orbit and repeat parameter combinations, indicating the applicability of such a mission to small, resource limited spacecraft. It is shown that a repeat ground-track can be achieved every 28 tidal periods with a single platform, through exploitation of natural perturbations alone (imager field of view would govern temporal resolution over any given region). A constellation of satellites could be deployed to achieve greater temporal resolution (additional satellites in an orbit plane) and greater number of ground-track repeats at specific tidal times (additional orbit planes). It is also shown that orbit parameters attributed to a repeat ground-track after exactly 57 tidal periods are almost identical to those required for a Sun-Synchronous orbit (approximately 5deg drift in relative solar angle per year). In this case, benefits from each class of synchronism could be exploited in order to achieve high quality, reliable visible imaging data at regular times in the tidal sequence.

KW - orbit determination

KW - remote sensing applications

KW - oceanic data

UR - http://www.iafastro.net/iac/paper/id/13924/summary.lite/.

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Lowe C, Macdonald M, Greenland SC, McKee D. Tidal synchronous orbit: A novel approach to remote sensing of oceanic regions. 2012. Poster session presented at 63rd International Astronautical Congress, Naples, Italy.