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REPUBLIC ACT 10913 or the ANTI-DISTRACTED DRIVING ACT(updated May 30, 2019)
1. What is RA 10913 or the Anti-Distracted Driving Act?
RA 10913 or the Anti-Distracted Driving Act (ADDA) is a law that prohibits a person who is driving a motor vehicle from holding and using mobile communication devices and electronic entertainment gadgets. The prohibition applies while the motor vehicle is in motion or temporarily stopped on a traffic light or an intersection.
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2. What vehicles are covered by this Act?
This law covers both public and private vehicles. It also covers wheeled agricultural machineries, construction equipment, and other forms of conveyances such as bicycles, pedicabs, trolleys, 'habal-habal', 'kuligligs', wagons, carriages, and carts that may either be human-powered or pulled by an animal as long as the same are operated or driven in public thoroughfares, highways or streets.
3. What does this law prohibit?
https://ajkpr-slots-france-demo-real-steel.peatix.com. Prohibited acts made while driving include but not limited to:
• Making or receiving calls
• Writing, sending or reading text-based communications
• Playing games
• Watching movies
• Performing calculations
• Reading e-books
• Composing messages
• Surfing or browsing the internet
4. Can a driver use his cellphone when he is stuck in traffic?
No. Even if a driver is stuck in traffic, as long as he is behind the wheel, he is still not allowed to hold and use his cellphone and/or gadget to make or receive calls; write, send or read text-based communications; play games; watch movies; perform calculations; read e-books; compose messages; surf or browse the internet; or other similar acts.
5. What are the actions exempted from this law?
Motorists are allowed to make or take emergency calls to authorities in cases of a crime, accidents, bomb or terrorist threat, fire or explosion, instances needing immediate medical attention, or when personal safety and security is compromised.
6. Can we use the hands-free function of our mobile communications device to make or receive calls?
Yes. Using the aid of a hands-free function such as speaker phones, earphones, Microphones or other similar device, which will allow a person to make and receive calls without holding his mobile communications device, is allowed.
However, using earphones to listen to music, or for other entertainment purposes, falls under 'similar acts' in Section 4(b) of the law.
7. Where can we mount our cellphones or GPS device?
GPS or cellphones may be placed or mounted below, at the same level, or on-top of the dashboard, and even on the windshield, as long as the highest point of the device is not higher than four (4) inches from the dashboard.
In the case of navigational apps, motorists are advised to set their destination prior to their departure. In cases when motorists need to find alternate routes while in traffic, they are advised to first pull their vehicles aside.
8. How about the use of dashcams? ls this covered by ADDA?
The use of dashcams is not covered by ADDA. To date, there is no legislation regulating the use of dashcams. However, for safety purposes, drivers are encouraged to mount their dashcams at the back of the rearview mirror.
9. Are we allowed to mount our cellphones on our motorcycles?
Yes, mounting of cellphones in handle bars or other parts of motorcycles is allowed, since this does not interfere with the driver's line of vision.
10. Does ADDA prohibit the mounting of other accessories in a vehicle's dashboard? How about engaging in other 'distracting activities'? Are these covered by the ADDA?
No. ADDA only covers the use of mobile communications devices and other electronic entertainment gadgets while vehicles are in motion or temporarily stopped on a traffic light or an intersection. It does NOT cover other accessories which may be found on your dashboard such as rosaries, tachometers, figurines, dashboard toys, crucifix, stickers, among others. Likewise, it does not cover activities such as putting make-up, drinking coffee, and other similar acts.
The best online slots. 11. Who are authorized to apprehend violating motorists?
The DOTr - Land Transportation Office (LTO), PNP-HPG, MMDA, and LGUs authorized to apprehend violators of the ADDA.
12. How will we know if drivers of private vehicles with heavily-tinted windshields are violating the law?
Aside from high-definition cameras that can monitor lights from devices inside heavily-tinted vehicles, the law will also be strictly enforced by enforcers on the ground who are trained to determine from the movement of the vehicle whether or not a driver commits distracted driving. A Memorandum Circular setting specifications on the regulation of tints shall also be released by LTO soon.
13. What are the penalties?
Violators will be penalized with a fine of five thousand pesos (Php5, 000) for the first offense, ten thousand pesos ((Php10, 000)) for the second offense, and fifteen thousand pesos ((Php15, 000)) for the third offense with a three-month suspension of driver's license.
Violations incurred beyond the third offense shall be penalized with the revocation of driver's license and a fine of twenty thousand pesos (Php20, 000).
14. Are operators of Public Utility Vehicles (PUV) also liable for violations made by drivers?
Yes. Operators and owners of Public Utility Vehicles (PUV) shall be held liable for the violations committed by their drivers.
15. Where to settle my violation?
Violators who were apprehended by LTO and/or PNP-HPG enforcers may settle their violations in the nearest LTO Office covering the area where they were apprehended. Adobe photoshop cc update download.
Violators apprehended by MMDA enforcers may either settle their violations thru selected Bayad Center within 7 days after they were issued a ticket. Violators may also pay their fines at the MMDA main office in Guadalupe, Makati City.
16. How about cyclists or those driving vehicles/machines that do not require licenses? How will they be apprehended?
Motorists who were caught violating the ADDA while riding a bicycle or wheeled agricultural machineries, construction equipment, and other forms of conveyances such as bicycles, pedicabs, trolleys, 'habal-habal', 'kuligligs', wagons, carriages, and carts that may either be human-powered or pulled by an animal, will still be apprehended, issued a ticket, and escorted up to the nearest authorized payment
center to settle his violation.
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However, if the driver does not have cash to pay for the fine, enforcers will have the authority to take the motorist's vehicle for safekeeping within a period of six (6)
months until the violator finally presents a receipt as proof of his payment of the fine.
Should the violator fail to settle his violation within six (6) months, the LTO shall have the authority to sell the impounded vehicle in favor of the government.
Perhaps the first quantitative investigation that can be said to have a direct bearing on the science of spectroscopy would be the discovery of Snel's law of refraction in about 1621. I am not certain, but I believe the original spelling of the Dutch mathematician who discovered the law was Willebrod Snel or Willebrord Snel, whose name was latinized in accordance with the custom of learned scholars of the day to Snellius, and later anglicized to the more familiar spelling Snell.
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Sir Isaac Newton's experiments were described in his Opticks of 1704. A most attractive illustration of the experiment, described in a work by Voltaire, is reproduced in Condon and Shortly's famous Theory of Atomic Spectra (1935). Newton showed that sunlight is dispersed by a prism into a band of colours, and the colours are recombined into white light when passed through an oppositely-oriented second prism. The infrared spectrum was discovered by Sir William Herschel in 1800 by placing thermometers beyond the red end of the visible spectrum. Johann Ritter the following year (and independently Wollaston) discovered the ultraviolet spectrum. In the period 1800-1803 Thomas Young demonstrated the wave nature of light with his famous double slit experiment, and he correctly explained the colours of thin films using the undulatory theory. Using Newton's measurements of this phenomenon, Young computed the wavelengths of Newton's seven colours and obtained the range (424) to (675 text{nm}). In 1802 William Wollaston discovered dark lines in the solar spectrum, but attached little significance to them.
In 1814 Joseph Fraunhofer, a superb instrument maker, made a detailed examination of the solar spectrum; he made a map of 700 of the lines we now refer to as 'Fraunhofer lines'. (Spectrum lines in general are sometimes described as 'Fraunhofer lines', but the term should correctly be restricted to the dark lines in the solar spectrum.) In 1817 he observed the first stellar spectra with an objective prism. He noted that planetary spectra resembled the solar spectrum, while many stellar spectra differed. Although the phenomenon of diffraction had been described as early as 1665 by Grimaldi, and Young had explained double-slit diffraction, Fraunhofer constructed the first diffraction grating by winding wires on two finely-cut parallel screws. With these gratings he measured the first wavelengths of spectrum lines, obtaining 588.7 for the line he had labelled D. We now know that this line is a close pair of lines of Na I, whose modern wavelengths are 589.0 and 589.6 nm. That different chemical elements produce their own characteristic spectra was noted by several investigators, including Sir John Herschel, (son of Sir William), Fox Talbot (pioneer in photography), Sir Charles Wheatstone (of Wheatstone Bridge fame), Anders Ångström (after whom the now obsolete unit the angstrom, Å, was named), and Jean Bernard Foucault (famous for his pendulum but also for many important studies in physical optics, including the speed of light) and especially by Kirchhoff and Bunsen. The fundamental quantitative law known as Kirchhoff's Law (see Chapter 2, section 2.4) was announced in 1859, and Kirchhoff and Bunsen conducted their extensive examination of the spectra of several elements. They correctly explained the origin of the solar Fraunhofer lines, investigated the chemical composition of the solar atmosphere, and laid the basic foundations of spectrochemical analysis. In 1868 Ångström published wavelengths of about 1000 solar Fraunhofer lines. In the 1870s, Rowland started to produce diffraction gratings of unparalleled quality and published extensive lists of solar wavelengths. New elements were being discovered spectroscopically:
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Cs, Rb, Tl (1860-61); In (1863); He (1868 - in the chromosphere of the solar spectrum at the instants of second and third contact of a solar eclipse, by Lockyer); Ga (1875); Tm (1870); Nd, Pr (1885); Sm, Ho (1886); Lu, Yb (1907).
Michelson measured the wavelength of three Cd I lines with great precision in 1893, and Fabry and Pérot measured the wavelengths of other lines in terms of the Cd I standards. For many years the wavelength of a cadmium lines was used as a basis for the definition of the metre.
Violators who were apprehended by LTO and/or PNP-HPG enforcers may settle their violations in the nearest LTO Office covering the area where they were apprehended. Adobe photoshop cc update download.
Violators apprehended by MMDA enforcers may either settle their violations thru selected Bayad Center within 7 days after they were issued a ticket. Violators may also pay their fines at the MMDA main office in Guadalupe, Makati City.
16. How about cyclists or those driving vehicles/machines that do not require licenses? How will they be apprehended?
Motorists who were caught violating the ADDA while riding a bicycle or wheeled agricultural machineries, construction equipment, and other forms of conveyances such as bicycles, pedicabs, trolleys, 'habal-habal', 'kuligligs', wagons, carriages, and carts that may either be human-powered or pulled by an animal, will still be apprehended, issued a ticket, and escorted up to the nearest authorized payment
center to settle his violation.
Beyond The Law: The Third Wave Mac Os Catalina
However, if the driver does not have cash to pay for the fine, enforcers will have the authority to take the motorist's vehicle for safekeeping within a period of six (6)
months until the violator finally presents a receipt as proof of his payment of the fine.
Should the violator fail to settle his violation within six (6) months, the LTO shall have the authority to sell the impounded vehicle in favor of the government.
Perhaps the first quantitative investigation that can be said to have a direct bearing on the science of spectroscopy would be the discovery of Snel's law of refraction in about 1621. I am not certain, but I believe the original spelling of the Dutch mathematician who discovered the law was Willebrod Snel or Willebrord Snel, whose name was latinized in accordance with the custom of learned scholars of the day to Snellius, and later anglicized to the more familiar spelling Snell.
Beyond The Law: The Third Wave Mac Os X
Sir Isaac Newton's experiments were described in his Opticks of 1704. A most attractive illustration of the experiment, described in a work by Voltaire, is reproduced in Condon and Shortly's famous Theory of Atomic Spectra (1935). Newton showed that sunlight is dispersed by a prism into a band of colours, and the colours are recombined into white light when passed through an oppositely-oriented second prism. The infrared spectrum was discovered by Sir William Herschel in 1800 by placing thermometers beyond the red end of the visible spectrum. Johann Ritter the following year (and independently Wollaston) discovered the ultraviolet spectrum. In the period 1800-1803 Thomas Young demonstrated the wave nature of light with his famous double slit experiment, and he correctly explained the colours of thin films using the undulatory theory. Using Newton's measurements of this phenomenon, Young computed the wavelengths of Newton's seven colours and obtained the range (424) to (675 text{nm}). In 1802 William Wollaston discovered dark lines in the solar spectrum, but attached little significance to them.
In 1814 Joseph Fraunhofer, a superb instrument maker, made a detailed examination of the solar spectrum; he made a map of 700 of the lines we now refer to as 'Fraunhofer lines'. (Spectrum lines in general are sometimes described as 'Fraunhofer lines', but the term should correctly be restricted to the dark lines in the solar spectrum.) In 1817 he observed the first stellar spectra with an objective prism. He noted that planetary spectra resembled the solar spectrum, while many stellar spectra differed. Although the phenomenon of diffraction had been described as early as 1665 by Grimaldi, and Young had explained double-slit diffraction, Fraunhofer constructed the first diffraction grating by winding wires on two finely-cut parallel screws. With these gratings he measured the first wavelengths of spectrum lines, obtaining 588.7 for the line he had labelled D. We now know that this line is a close pair of lines of Na I, whose modern wavelengths are 589.0 and 589.6 nm. That different chemical elements produce their own characteristic spectra was noted by several investigators, including Sir John Herschel, (son of Sir William), Fox Talbot (pioneer in photography), Sir Charles Wheatstone (of Wheatstone Bridge fame), Anders Ångström (after whom the now obsolete unit the angstrom, Å, was named), and Jean Bernard Foucault (famous for his pendulum but also for many important studies in physical optics, including the speed of light) and especially by Kirchhoff and Bunsen. The fundamental quantitative law known as Kirchhoff's Law (see Chapter 2, section 2.4) was announced in 1859, and Kirchhoff and Bunsen conducted their extensive examination of the spectra of several elements. They correctly explained the origin of the solar Fraunhofer lines, investigated the chemical composition of the solar atmosphere, and laid the basic foundations of spectrochemical analysis. In 1868 Ångström published wavelengths of about 1000 solar Fraunhofer lines. In the 1870s, Rowland started to produce diffraction gratings of unparalleled quality and published extensive lists of solar wavelengths. New elements were being discovered spectroscopically:
Beyond The Law: The Third Wave Mac Os 7
Cs, Rb, Tl (1860-61); In (1863); He (1868 - in the chromosphere of the solar spectrum at the instants of second and third contact of a solar eclipse, by Lockyer); Ga (1875); Tm (1870); Nd, Pr (1885); Sm, Ho (1886); Lu, Yb (1907).
Michelson measured the wavelength of three Cd I lines with great precision in 1893, and Fabry and Pérot measured the wavelengths of other lines in terms of the Cd I standards. For many years the wavelength of a cadmium lines was used as a basis for the definition of the metre.
Although the existence of ultraviolet radiation had been detected by Richter, the first person actually to see an ultraviolet (UV) spectrum was Sir George Stokes (of viscosity and fluorescence fame), using a quartz prism (ordinary glass absorbs UV) and a fluorescent uranium phosphate screen. In 1906 Lyman made extensive investigations into ultraviolet spectra, including the hydrogen series now known as the Lyman series. Langley invented the bolometer in 1881, paving the way to the investigation of infrared spectra by Paschen. Balmer published his well-known formula for the wavelengths of the hydrogen Balmer series in 1885. Power rangers lightspeed rescue mac os. Zeeman discovered magnetic splitting in 1896. Bohr's theory of the hydrogen atom appeared in 1913, and the wave mechanics of Schrödinger was developed in the mid 1920s.
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