geosc040, lecture 23. tides: sun, moon, rise and fall and sealevel changes

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Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

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Page 1: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall

and Sealevel Changes

Page 2: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Do you find yourself dreaming about the ocean?

Join the Marine Science Society!! (MSS)Meeting Time: Bi-weekly, Thursday at 6 pm in 103 Ferguson

Next meeting: April 17th For more information email Meredith Fish at: [email protected]

Check out our Facebook page: Penn State Marine Science Society

http://www.cpa.psu.edu/news/candy-wrapper-collection-2013%E2%80%932014

Page 3: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Read Chapter 9!

Check it out!Course web site:

Apr 15, 2014 Total Lunar Eclipse

Sargasso Sea Tribute & Declaration

Quiz 2: On Apr. 14

OLA 11 Due today, Thursday, 10 Apr

Homework 4 due Apr. 22http://www3.geosc.psu.edu/geosc040/Syllabus.html

Extra Credit Letter Grades will be posted by ~Apr 24

Page 4: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

http://vimeo.com/89868953

North Atlantic stock: spawn in Sargasso Sea then larvae migrate to freshwater

Page 5: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Spawning Behavior• Catadromous vs. Anadromous Fishes

– anadromous, lit. means ‘running upward’– ”down-wandering” vs. “up-wandering” to spawn– eels--catadromous

• Salmon, shad, herring, striped bass, etc. are anadromous. They migrate from saltwater to freshwater to spawn

• Think about how they must “switch over” in fluid regulation• Note: Pacific salmon shrink and resorb their intestinal system when

they are about to spawn (they die shortly after spawning, of course)

Shad

Anadromous Fish

Page 6: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Origin of TidesTwo Approaches

1) Equilibrium theory. Makes simplifying assumptions, provides a basic understanding of tides

2) Dynamic theory. Complexities of coastlines, bays, ocean basin geometry, Earth deformation.

Page 7: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Fig 10.13

Fig 10.14Global Distribution of Tide Types

Note dominance of Semidiurnal tides

Page 8: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Tidal Regimes Macrotidal

Mont St. Michel, France

Page 9: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Why are there Two Tidal Bulges!-Gravity and Inertia (centrifugal force)

Gravity

Inertia

Page 10: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Why are there Two Tidal Bulges!-Gravity and Inertia (centrifugal force)

http://www.fearofphysics.com/SunMoon/sunmoon1.html

Page 11: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Why are there Two Tidal Bulges!-Gravity and Inertia (centrifugal force)

Page 12: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Fig 10.12

Basic elements of tidal variation over one month

Page 13: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes
Page 14: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes
Page 15: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Note Asymmetry in highs and lows

Page 16: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Note Asymmetry in highs and lows

A Higher High Tide

Lower High Tide

Page 17: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Timing and Predictability of Tides• Semidiurnal tides have a range that cycles over a 14 day period. • This coincides with the moon’s 28 day orbital period.• Monthly inequality• Max semi-diurnal tides occur when spring tides coincide with lunar perigee.

Predicting tides is difficult Factors to consider:

• lunar distance• solar distance• lunar declination• solar apparent declination• relative alignment of sun

and moon• coastal morphology• location of amphidromic

point• must also take into account

storms, wind patterns, etc.

Page 18: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

This shows a situation when ______ occur, which is the time of the month when tides are ______…

A. Spring Tides, Largest because the Sun and Moon act togetherB. Spring Tides, Smallest because the Sun and Moon act in opposite

directionsC. Neap Tides, Smallest because the Sun and Moon act in opposite

directionsD. Neap Tides, Largest because the Sun and Moon act together

Page 19: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

A. This diagram shows the time of the month when tides have largest amplitude (spring tides).

B. This diagram shows the time of the month when tides are smallest amplitude (neap tides).

C. Centrifugal forces play a role in creating ocean tides.D. The Earth-Moon system revolves around a point that is within

EarthE. All but A

Which of the following are true

Page 20: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Timing and Predictability of Tides• Semidiurnal tides have a range that cycles over a 14 day period. • This coincides with the moon’s 28 day orbital period.• Monthly inequality• Max semi-diurnal tides occur when spring tides coincide with lunar perigee.

Predicting tides is difficult Factors to consider:

• lunar distance• solar distance• lunar declination• solar apparent declination• relative alignment of sun

and moon• coastal morphology• location of amphidromic

point• must also take into account

storms, wind patterns, etc.

Page 21: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Variations in tidal amplitude

• Moon’s orbit around Earth is elliptical (eccentricity ~0.055)

Apogee (farthest ~0.40x106 km)

Perigee (closest ~0.36x106 km)

• Difference (4 x104 km) is important because gravitational attraction is proportional to square of distance

• Declination of lunar orbit varies 28.5 degrees above and below equator during lunar month

ApogeePerigee

Page 22: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Note that the Spring Tide during days 22 through 26 is bigger than the Spring Tide during days 6-8.

ApogeePerigee

• Max semi-diurnal tides occur when spring tides coincide with lunar perigee.

• Moon’s orbit around Earth is elliptical

Apogee (farthest ~0.40x106 km)

Perigee (closest ~0.36x106 km)

Page 23: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

The tidal bulges on Earth:A. Are fixed relative to Earth’s surface, so they rotate 360° during a

day just like everything on EarthB. Make half a revolution each day, which is why there are two

bulges.C. Rotate from the north pole to the south pole and back every 24

hours.D. Are always directly over the equator.E. none of the above

Page 24: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

The tidal bulges on Earth:A. Are fixed relative to Earth’s surface, so they rotate 360° during a

day just like everything on EarthB. Make half a revolution each day, which is why there are two

bulges.C. Rotate from the north pole to the south pole and back every 24

hours.D. Are always directly over the equator.E. none of the above• The tidal bulges are

‘stationary’ relative to the position of the moon and sun

• Points on Earth’s surface rotate under the high-tide bulges and low tide regions

Page 25: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

The tidal bulges on Earth:A. Are fixed relative to Earth’s surface, so they rotate 360° during a

day just like everything on EarthB. Make half a revolution each day, which is why there are two

bulges.C. Rotate from the north pole to the south pole and back every 24

hours.D. Are always directly over the equator.E. none of the above

Page 26: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

The Spring Tide during days 22 through 26 is bigger than the Spring Tide during days 6-8. What could explain this?

A) The Sun is closer to the moon

B) The moon is closer to Earth

C) Earth is spinning faster then

D) Tides are always larger at new moon

• Semidiurnal tides have a range that cycles over a 14 day period.

• This coincides with the moon’s 28 day orbital period.

• Max semi-diurnal tides occur when spring tides coincide with lunar perigee.

Page 27: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

The Spring Tide during days 22 through 26 is bigger than the Spring Tide during days 6-8. What could explain this?

A) The Sun is closer to the moon

B) The moon is closer to Earth

C) Earth is spinning faster then

D) Tides are always larger at new moon

ApogeePerigee

• Max semi-diurnal tides occur when spring tides coincide with lunar perigee.

Page 28: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Diurnal and semi-diurnal Variations in tidal amplitude

Page 29: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Note that high tides are not always of equal amplitude. Which of the following are true?

A) Point x in the figure could have this tidal record

B) The difference (asymmetry) in high tides would be larger for points at higher latitude than point x

C) Tides are always larger at new moon

D) A and B

x

Page 30: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Note that high tides are not always of equal amplitude. Which of the following are true?

A) Point x in the figure could have this tidal record

B) The difference (asymmetry) in high tides would be larger for points at higher latitude than point x

C) Tides are always larger at new moon

D) A and B x

Page 31: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Origin of TidesTwo Approaches

1) Equilibrium theory. Makes simplifying assumptions, provides a basic understanding of tides

2) Dynamic theory. Complexities of coastlines, bays, ocean basin geometry, Earth deformation.

Page 32: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Dynamic theory of Tides and Amphidromic points

Continental margins and the Coriolis effect

1) Continents. As Earth spins the tidal bulges attempt to stay below the moon and opposite of it. Therefore water is forced against the continental margin.

•This occurs on the western margin of the ocean basin (eastern margin of continent)

Page 33: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Dynamic theory of Tides and Amphidromic points

Continental margins and the Coriolis effect

1) Continents. As Earth spins the tidal bulges attempt to stay below the moon and opposite of it. Therefore water is forced against the continental margin.

•This occurs on the western margin of the ocean basin (eastern margin of continent)

• Tides are very long-wavelength shallow water waves.

• Tidal crests are separated by half of Earth’s circumference!

• Picture waves trapped in ocean basins between continents.

2) Coriolis. In the northern hemisphere, as water travels north it moves to the right and thus the Eastern side of the ocean basin. The opposite happens for water traveling south.

•This sets up a counterclockwise wave motion, with water sloshing back and forth in the ocean basins.

Page 34: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Dynamic theory of Tides and Amphidromic points

1) Continents. As Earth spins the tidal bulges attempt to stay below the moon and opposite of it. Therefore water is forced against the continental margin.

•This occurs on the western margin of the ocean basin (eastern margin of continent)

• Tides are very long-wavelength shallow water waves.

• Tidal crests are separated by half of Earth’s circumference!

• Picture waves trapped in ocean basins between continents.

Page 35: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Dynamic theory of Tides and Amphidromic points

Continental margins and the Coriolis effect

Development of Amphidromic Circulation

Page 36: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Dynamic theory of Tides and Amphidromic points

Continental margins and the Coriolis effect

Development of Amphidromic Circulation

Page 37: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Amphidromic CirculationTidal crests move in a

counter-clockwise pattern around the basins of the northern hemisphere.

Like Fig 10.17

Noon

3 pm

6 pm

9 pm

Page 38: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Development of Amphidromic CirculationTidal crests move in a

counter-clockwise pattern around the basins of the northern hemisphere.

These rotary waves revolve around a fixed NODE (which experiences no tidal fluctuation-an amphidromic point).

The resulting circulation is called an amphidromic system.

Page 39: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Amphidromic Circulation and Tides

Page 40: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Amphidromic Circulation

These rotary waves revolve around a fixed NODE (which experiences no tidal fluctuation-an amphidromic point).

The resulting circulation is called an amphidromic system.

Tidal crests move in a counter-clockwise pattern around the basins of the northern hemisphere.

Page 41: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

The tidal range toward the center of an amphidromic system is ____ the range at the edges of the system.

A. of longer duration thanB. larger thanC. about the same asD. smaller thanE. none of the above.

Page 42: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Development of Amphidromic CirculationTidal crests move in a

counter-clockwise pattern around the basins of the northern hemisphere.

These rotary waves revolve around a fixed NODE (which experiences no tidal fluctuation-an amphidromic point).

The resulting circulation is called an amphidromic system.

Page 43: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Amphidromic Circulation

Earth has about 12 amphidromic systems

• Tidal amplitude increases progressively away from amphidromic points

Fig 10.16

Page 44: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

The dynamic theory of tidesA. Accounts for ocean basin geometry and continentsB. Predicts that tides move as shallow water wavesC. Accounts for the Coriolis effectD. All of the aboveE. None of the above

Page 45: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

For an amphidromic system such as shown, if there is a high tide at B, there will be a high tide at A roughly

A. 12 hours laterB. 2 hours laterC. 6 hours laterD. At the same timeE. 3 hours later

B

A

Assume a semi-diurnal system

Page 46: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

For an amphidromic system such as shown, if there is a high tide at B, there will be a high tide at B roughly

A. 12 hours laterB. 2 hours laterC. 6 hours laterD. At the same timeE. 3 hours later

B

A

Assume a semi-diurnal system

Page 47: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

http://www.die.net/earth/hemisphere.html

Page 48: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Tides are shallow water waves, produced by gravity and inertial (centrifugal) forces

A tide is a “forced” wave, and actually must travel very rapidly to keep up with the forcing (forcing is as fast as 1600 km/hr. at equator)

Earth-Moon Rotation AxisREVIEW

Page 49: Geosc040, Lecture 23. Tides: Sun, Moon, Rise and Fall and Sealevel Changes

Dynamic theory of Tides. Complexities of coastlines, bays, ocean basin geometry, Earth deformation.